October 9

A New Star Changes the Heavens

1604 — A Brilliant New Star Appears in the Milky Way

Evening; precise time not established

On the evening of October 9, 1604, Italian astronomer Ilario Altobelli looked toward a striking gathering of planets in the constellation Ophiuchus. Mars, Jupiter, and Saturn were close together in the sky. Altobelli had been watching the region carefully. Now something was different. There was another brilliant point of light. A new star had appeared. Today we know that Altobelli was witnessing a supernova—the catastrophic destruction of a star roughly 20,000 light-years from Earth. It became known as Kepler's Supernova, or SN 1604. It remains the most recent supernova known to have been observed occurring in our own Milky Way galaxy. Altobelli's role deserves particular attention. The supernova carries Johannes Kepler's name, which can easily create the impression that Kepler discovered it. He did not. Historical evidence indicates that Altobelli observed the new object in northern Italy on October 9. Other observers soon reported it independently. In Prague, Johannes Brunowski noticed it on October 10 and brought it to Kepler's attention. Cloudy weather prevented Kepler from seeing it himself until October 17. Once he did, however, Kepler studied the object extensively. His careful observations and subsequent publication made his name permanently associated with the event. The new star was impossible to ignore. It eventually became brighter than Jupiter and remained visible to the unaided eye for many months. At its brightest, it could even be seen during daylight. For seventeenth-century astronomy, the event presented a profound question. Where was it? The answer mattered because European natural philosophy was still heavily influenced by the cosmology of Aristotle. In the traditional Aristotelian universe, the region below the Moon was a realm of change. Things were born. Things decayed. Things moved and transformed. But beyond the Moon lay the supposedly perfect and unchanging heavens. Stars belonged to that eternal celestial realm. A genuinely new star would therefore be deeply troublesome. One possibility was that the object was not actually among the stars at all. Perhaps it was a phenomenon in Earth's atmosphere. Astronomers could test that possibility using parallax. A nearby object viewed from different locations should appear to shift relative to the distant stars. The new object showed no measurable parallax with the instruments available. That placed it far beyond the Moon. Something in the supposedly unchanging heavens had changed. This was not the first time such evidence had appeared. In 1572, Tycho Brahe had studied another brilliant “new star”—also a supernova—and similarly found no measurable parallax. The great comet of 1577 had further undermined the traditional idea that the celestial spheres were solid, immutable structures. SN 1604 added another powerful piece of evidence. The heavens were not changeless. Kepler followed the object as its brightness evolved and published his observations in 1606 in a work commonly known by its shortened title, De Stella Nova—On the New Star. The telescope had not yet entered astronomy. Galileo's telescopic observations would begin only a few years later. Everything astronomers learned about the new star in 1604 therefore came from careful naked-eye observation, positional measurement, and reasoning. They could not know what the object physically was. The nature of supernovae would remain unknown for centuries. Today astronomers identify SN 1604 as a Type Ia supernova. Such explosions involve white dwarfs—extremely dense stellar remnants—in binary systems. A thermonuclear runaway destroys the white dwarf, releasing an enormous amount of energy. The original explosion is long over. But it left something behind. An expanding shell of gas and energetic particles known as Kepler's Supernova Remnant still occupies the region. Modern observatories examine that remnant at wavelengths Altobelli and Kepler could never have imagined. Visible-light telescopes study its glowing structures. Radio telescopes examine energetic particles and magnetic fields. Infrared observatories investigate heated dust. X-ray telescopes reveal gas heated to millions of degrees by the expanding shock wave. Four centuries after the new star appeared, the explosion is still teaching us about the deaths of stars. There is also a humbling perspective hidden within the date. The supernova did not actually explode in 1604. Because it lies roughly 20,000 light-years away, the light that reached Earth that October had been traveling through the Milky Way for approximately 20,000 years. The explosion had occurred long before recorded human history. October 9, 1604, marks not when the star exploded, but when news of that explosion finally reached human eyes.

Why It Matters: SN 1604 is the most recent supernova known to have been observed occurring in the Milky Way. Its appearance provided further evidence that the heavens were not perfect and unchanging, helping undermine an ancient cosmological assumption just before telescopic astronomy transformed humanity's understanding of the universe. The surviving remnant remains an important astronomical laboratory more than four centuries later.

 

Also on This Day

1992 — The Peekskill Meteorite Hits a Parked Car

Fireball observed approximately 23:48 UTC

On the evening of October 9, 1992, spectators at high-school football games across the eastern United States noticed something extraordinary moving through the sky. A brilliant fireball streaked overhead. Unlike most meteors of its era, however, this one had an unusually large audience equipped with video cameras. The result was one of the best-recorded meteor events in history up to that time. The object entered Earth's atmosphere over the eastern United States and traveled northeastward in a long luminous trajectory. Thousands of people saw it. At least 16 independent videos recorded portions of its passage. Those recordings became scientifically valuable. Because the meteor had been photographed from multiple locations, researchers could reconstruct its atmospheric trajectory and estimate the orbit it had followed around the Sun before encountering Earth. But the most famous part of the story happened on the ground. In Peekskill, New York, 18-year-old Michelle Knapp heard a loud crash outside her home. A rock from space had struck her parked 1980 Chevrolet Malibu. The meteorite punched through the rear of the car, leaving a large dent and a hole, before coming to rest beneath it. The recovered stone weighed approximately 12.4 kilograms—more than 27 pounds. It was identified as an H6 ordinary chondrite, part of one of the most common broad classes of stony meteorites. The car quickly became almost as famous as the meteorite. But scientifically, the videos were more important. Meteorites are pieces of asteroids that survive atmospheric passage and reach the ground. Usually, scientists can analyze the recovered stone but have limited information about precisely how that particular object traveled through the solar system before falling. Peekskill provided both. The videos documented the atmospheric trajectory. The meteorite provided the physical sample. Researchers could therefore connect a laboratory specimen with information about the orbit of its parent meteoroid before it encountered Earth. The event anticipated a connection we encountered only two days ago with 2008 TC3. In 1992, cameras recorded a meteorite-producing object primarily as it traveled through Earth's atmosphere. In 2008, astronomers detected 2008 TC3 before it entered the atmosphere and predicted its impact. Together, such events show how asteroid astronomy, meteor science, orbital mechanics, and laboratory analysis increasingly became parts of the same field.

Why It Matters: The Peekskill meteorite became one of the best-documented meteorite falls of its time because its brilliant atmospheric passage was recorded on numerous independent videos and a substantial fragment was recovered. Those observations allowed scientists to connect a meteorite studied in the laboratory with the trajectory of the object that delivered it to Earth.

2009 — LCROSS Strikes the Moon and Finds Water

Centaur impact: 11:31:19.51 UTC
LCROSS impact: 11:35:34 UTC

On October 9, 2009, NASA deliberately crashed a rocket into the Moon. Four minutes later, it crashed a spacecraft nearby. This was not a failure. It was the experiment. The Lunar Crater Observation and Sensing Satellite—LCROSS—had been launched with the Lunar Reconnaissance Orbiter on June 18, 2009. Its principal question was one of enormous importance for lunar science and future exploration: Is there water ice in the permanently shadowed craters near the Moon's poles? For most of the twentieth century, the Moon was widely imagined as almost completely dry. But spacecraft observations had gradually complicated that picture. Radar and neutron measurements provided evidence suggesting that hydrogen-rich material—and possibly water ice—might exist near the lunar poles. There was a reason to look there. Because the Moon's rotational axis is only slightly tilted, sunlight never reaches the floors of some deep craters near the poles. These permanently shadowed regions can remain extraordinarily cold. For billions of years, they may have acted as cold traps, preserving volatile substances delivered by comets and asteroids or produced through other processes. LCROSS was designed to look inside one. The target was Cabeus crater, near the lunar south pole. The mission used an ingenious approach. The spent Centaur upper stage that had helped launch LCROSS was retained as an impactor. At 11:31:19.51 UTC, the roughly two-ton Centaur slammed into the permanently shadowed floor of Cabeus. The impact excavated hundreds of tons of lunar material and threw part of it upward. Material that may have remained in darkness for billions of years suddenly rose into sunlight. LCROSS followed approximately four minutes behind. Its cameras and spectrometers watched the impact and examined the resulting plume. Then the spacecraft flew directly through the debris. It transmitted its measurements to Earth until, at 11:35:34 UTC, LCROSS itself struck the Moon. The mission was over. The analysis was just beginning. The visible plume proved less dramatic than many observers had expected. But LCROSS's instruments had obtained the measurements that mattered. On November 13, NASA announced the result: water had been detected. Subsequent analysis strengthened and expanded the conclusion. The excavated material contained water and other volatile substances. Later measurements indicated that some lunar polar deposits contained grains of relatively pure water ice. The Moon was not simply the bone-dry world once imagined. Its permanently shadowed regions preserved a chemically rich record. The discovery had implications extending beyond lunar geology. Water is useful. Future explorers could potentially use lunar ice for drinking water. Water can be separated into hydrogen and oxygen, potentially providing breathable oxygen and ingredients for rocket propellant. Whether particular deposits can practically and responsibly be used remains a question for future exploration. But the presence of accessible lunar water fundamentally changes discussions about sustained activity on the Moon.

Why It Matters: LCROSS provided direct evidence of water in a permanently shadowed crater near the Moon's south pole. The discovery transformed scientific understanding of lunar volatiles and helped establish the polar regions as some of the most important locations for future lunar science and exploration.

 

The Bigger Picture

October 9 is a day about things that were present before we understood they were there. SN 1604 suddenly appeared in the night sky. But the star had actually exploded thousands of years earlier. The light simply had not reached Earth yet. The Peekskill meteoroid traveled through the solar system before intersecting Earth's orbit. Human beings became aware of it only when the atmosphere turned its arrival into a brilliant streak of light. Water had probably existed in the permanently shadowed regions of the Moon for immense spans of time before LCROSS excavated some of it into sunlight. In every case, discovery did not create the phenomenon. Discovery changed our awareness of it. That distinction lies at the heart of astronomy. The universe does not reveal itself according to the timetable of human understanding. Stars explode whether anyone is watching. Asteroids cross planetary orbits whether anyone has discovered them. Ice accumulates in darkness whether anyone has sent a spacecraft to look. Science gives us ways to notice what was already there. There is another progression across the three events. In 1604, astronomers possessed their eyes and geometry. In 1992, video cameras captured a meteor from many different locations, allowing computers and mathematics to reconstruct its path. In 2009, scientists did something more active. They deliberately performed an experiment on another world. LCROSS did not merely observe the Moon. It struck the surface in a carefully selected location so that buried material would be exposed and measured. Astronomy had evolved from observing what the universe presented to us into designing experiments on worlds beyond Earth. And yet the basic motivation remained the same. There was something we did not know. So we found a way to look.

At a Glance

1604 — Evening; precise time not established — Ilario Altobelli makes the earliest known reported observation of the brilliant new star now called SN 1604 or Kepler's Supernova, the most recent supernova known to have been observed occurring in the Milky Way.

1992 — Approximately 23:48 UTC — The Peekskill fireball crosses the eastern United States; a 12.4-kilogram meteorite fragment subsequently strikes a parked automobile in Peekskill, New York.

2009 — 11:31:19.51 UTC — LCROSS's Centaur upper stage impacts Cabeus crater near the Moon's south pole, excavating material from a permanently shadowed region.

2009 — 11:35:34 UTC — The LCROSS shepherding spacecraft, after observing and passing through the Centaur's debris plume, impacts the Moon; its measurements subsequently confirm the presence of lunar water.

October 8

Finding Order Among the Stars

1873 — Ejnar Hertzsprung Is Born

Time unknown

On October 8, 1873, Ejnar Hertzsprung was born in Frederiksberg, Denmark, near Copenhagen. His name would eventually become attached to one of the most important diagrams in all of astronomy. The Hertzsprung-Russell diagram looks deceptively simple. Place stars according to their luminosity on one axis. Place them according to surface temperature—or a closely related measure such as color or spectral type—on the other. Then something remarkable happens. The stars do not scatter randomly across the diagram. They form patterns. Those patterns reveal the life stories of stars. Hertzsprung did not begin his career as a professional astronomer. He trained as a chemical engineer at the Polytechnic Institute in Copenhagen and subsequently worked in St. Petersburg and studied photochemistry in Leipzig. Photography helped draw him toward astronomy. By the early twentieth century, astronomers had accumulated enormous amounts of information about stars. Spectroscopy allowed them to divide stars into spectral classes according to the absorption lines in their light. Photography allowed increasingly precise measurements of stellar brightness and position. But an important question remained: What did these classifications actually tell astronomers about the physical nature of stars? Hertzsprung recognized that stars with similar spectra could nevertheless possess very different intrinsic luminosities. Some were enormously luminous. Others were comparatively faint. In papers published in 1905 and 1907, he distinguished between what came to be called giant and dwarf stars. The distinction was profound. Two stars could have approximately the same surface temperature and therefore similar colors and spectra, yet one could radiate vastly more energy than the other because it was physically much larger. Hertzsprung began examining the relationship between stellar color and absolute brightness. When he plotted stars according to these properties, patterns appeared. Independently, American astronomer Henry Norris Russell approached the same relationship from another direction and developed a similar graphical representation. The resulting relationship became known as the Hertzsprung-Russell diagram, usually abbreviated the H-R diagram. Its importance is difficult to overstate. Most ordinary stars occupy a broad diagonal band called the main sequence. Hot, luminous stars appear toward one end. Cooler, fainter stars appear toward the other. Our Sun lies on this main sequence. But not all stars do. Giants and supergiants occupy regions of much greater luminosity. White dwarfs occupy a region containing hot but faint stars—objects whose high temperatures are combined with extremely small physical sizes. At first, the diagram was principally an empirical relationship. Astronomers could see that stars occupied different regions. As stellar astrophysics developed, however, the reason became clearer. The H-R diagram is, in effect, a map of stellar evolution. A star spends most of its life on the main sequence, generating energy by fusing hydrogen into helium in its core. When the core hydrogen becomes depleted, the star changes. Its internal structure adjusts. It may expand into a red giant. Depending upon its mass, later stages can carry it toward a white dwarf, supernova explosion, neutron star, or black hole. Star clusters made the diagram even more powerful. Because stars within a cluster generally formed at approximately the same time and lie at approximately the same distance from Earth, astronomers could compare their positions on the H-R diagram and determine where stars of different masses had begun leaving the main sequence. That main-sequence turnoff became an important method for estimating the ages of star clusters. Hertzsprung also made important contributions to the study of variable stars and stellar distances. He recognized the importance of Henrietta Swan Leavitt's discovery of the period-luminosity relationship among Cepheid variable stars and helped apply that relationship to the astronomical distance scale. He also became an expert in the photographic study of double stars. In 1919, Hertzsprung joined the Leiden Observatory in the Netherlands. He became its director in 1935 and remained there until his retirement in 1944. By then, the diagram bearing his and Russell's names had become one of astronomy's essential tools. It remains so today. Modern astronomers may use exquisitely precise measurements from spacecraft such as Gaia, sophisticated stellar models, and computers capable of analyzing millions or billions of stars. Yet one of the first things they can do with those measurements is remarkably familiar: plot luminosity against temperature or color. The patterns Hertzsprung helped recognize more than a century ago immediately appear.

Why It Matters: Ejnar Hertzsprung helped reveal that stars are not a random assortment of lights but members of physically meaningful populations. The Hertzsprung-Russell diagram became one of astronomy's fundamental tools, allowing astronomers to connect a star's temperature and luminosity with its size, age, and evolutionary state. It transformed stellar classification into a way of understanding the lives of stars.

 

Also on This Day

1992 — Pioneer Venus Orbiter Sends Its Final Transmission

19:22 UTC

On October 8, 1992, a spacecraft that had been designed to operate around Venus for less than a year sent its final message home. It had survived for almost fourteen years. NASA's Pioneer Venus Orbiter, also known as Pioneer Venus 1, had launched in May 1978 and entered orbit around Venus on December 4 of that year. It became the first American spacecraft to orbit Venus. The mission was originally expected to operate for approximately one Venusian rotation—about 243 Earth days. Instead, Pioneer Venus continued observing the planet year after year. Venus presents a particularly difficult problem for planetary scientists. Its surface is hidden beneath a global layer of thick clouds. Visible-light telescopes cannot simply photograph its mountains, plains, and other surface features from orbit. Pioneer Venus therefore carried radar. By transmitting radio waves through the clouds and measuring the echoes returning from the surface, scientists could begin reconstructing the topography below. The spacecraft eventually mapped most of Venus within the latitudes accessible to its radar. Its observations revealed an enormous landscape of plains, highlands, mountains, and other geological structures. Among the most prominent was Maxwell Montes, the highest mountain range on Venus, rising roughly 11 kilometers above the planet's mean surface level. But Pioneer Venus was much more than a radar mapper. Its instruments studied the planet's atmosphere, clouds, ionosphere, magnetic environment, and interaction with the solar wind. The spacecraft helped establish that Venus lacks a strong intrinsic global magnetic field comparable to Earth's. That difference matters. Earth's magnetic field carves out a vast magnetosphere around our planet. Venus instead interacts much more directly with the stream of charged particles flowing outward from the Sun. Pioneer Venus repeatedly crossed the resulting boundaries and allowed scientists to study that interaction over many years. Its ultraviolet observations revealed changing patterns in Venus's cloud tops. Other measurements investigated the composition and structure of the upper atmosphere. The spacecraft also detected evidence associated with lightning in the Venusian atmosphere. Its longevity created another scientific advantage. Fourteen years of observations allowed researchers to study Venus through changing conditions in the solar cycle. A mission intended to provide a snapshot became a long-term observatory. By the early 1990s, another NASA spacecraft had arrived. Magellan entered Venus orbit in 1990 carrying a much more sophisticated radar system and began mapping the planet at dramatically higher resolution. Pioneer Venus was no longer alone. But the older spacecraft continued working. Mission controllers used its dwindling propellant carefully, adjusting its orbit and allowing it to descend progressively closer to the upper atmosphere. Those final low-altitude passes provided measurements from regions the spacecraft had not previously sampled. Eventually, there was no propellant left to maintain the orbit. At 19:22 UTC on October 8, 1992, NASA received Pioneer Venus Orbiter's final transmission. Soon afterward, the spacecraft entered the dense Venusian atmosphere and was destroyed. A mission designed for roughly eight months had lasted almost fourteen years.

Why It Matters: Pioneer Venus Orbiter transformed knowledge of Earth's nearest planetary neighbor through long-term measurements of its atmosphere, clouds, plasma environment, and hidden surface. Its extraordinary longevity allowed scientists to observe Venus across much of a solar cycle, turning a short planned mission into one of the enduring successes of early planetary exploration.

 

The Bigger Picture

October 8 brings together two very different ways of understanding distant objects. Hertzsprung could not travel to a star. Pioneer Venus could travel to Venus. That difference illustrates one of the central divisions within astronomy and space science. For the stars, distance forces us to become extraordinarily skilled at interpreting light. From a point of light, astronomers can determine temperature. From spectral lines, they can infer chemical composition. From brightness and distance, they can calculate luminosity. From patterns among millions of stars, they can reconstruct stellar evolution. Hertzsprung helped demonstrate the power of putting those measurements together. A star's position on the H-R diagram tells a story. For planets within our own solar system, however, humanity eventually gained another possibility. We could send instruments there. Venus had been observed from Earth for thousands of years. Telescopes showed its phases. Spectroscopy provided clues about its atmosphere. Radar observations from Earth penetrated its clouds. But spacecraft such as Pioneer Venus could make sustained measurements from the planet itself—orbiting above its atmosphere, repeatedly sampling its environment, and transmitting the results home. These two methods are not competitors. They are parts of the same scientific process. Astronomy teaches us how much can be learned from a distance. Space exploration allows us, where possible, to go closer and test what we think we know. There is another connection between the two events. Both depended upon finding patterns over time. Hertzsprung found order among apparently different stars. Pioneer Venus survived long enough to watch Venus interact with a changing Sun over much of a solar cycle. A single observation can reveal something important. A collection of observations can reveal a system. And systems are what science ultimately seeks to understand. The H-R diagram turned thousands of stars into a coherent story of stellar lives. Fourteen years at Venus turned countless measurements into a changing portrait of a planet. October 8 therefore reminds us that one of the great powers of astronomy is not merely seeing farther. It is learning how to recognize order in what we see.

At a Glance

1873 — Time unknown — Ejnar Hertzsprung is born near Copenhagen, Denmark; his work relating stellar color, temperature, and luminosity will help produce the Hertzsprung-Russell diagram, one of the fundamental tools of stellar astronomy.

1992 — 19:22 UTC — NASA receives the final transmission from Pioneer Venus Orbiter after nearly fourteen years of observations around Venus, ending a mission originally designed to last only about eight months.

October 7

Humanity Sees the Other Side of the Moon

1959 — Luna 3 Photographs the Far Side of the Moon

First photograph: 03:30 UTC

On October 7, 1959, humanity saw a landscape that had remained hidden throughout all previous human history. It was the other side of the Moon. At 03:30 UTC, the Soviet spacecraft Luna 3 began photographing the lunar far side. The accomplishment was remarkable not simply because of the distance involved, but because of a fundamental characteristic of the Moon's motion. The Moon rotates on its axis. But it takes approximately the same amount of time to rotate once as it takes to orbit Earth once. This condition, called synchronous rotation, causes nearly the same lunar hemisphere always to face Earth. Small oscillations known as libration allow observers to see somewhat more than half of the lunar surface over time. But a large portion of the Moon remained permanently hidden from direct observation on Earth. Generations of astronomers could map craters, mountains, and dark volcanic plains on the familiar lunar face. No telescope, regardless of its power, could look around the Moon and show what lay beyond its edge. To see the far side, humanity would have to send a camera there. Luna 3 did exactly that. The spacecraft had launched on October 4 and swept past the Moon's southern polar region on October 6. Its trajectory then carried it behind the Moon and outward, placing its cameras in position to look back at the illuminated far hemisphere. At 03:30 UTC on October 7, from a distance of roughly 63,500 kilometers from the lunar surface, the photographic sequence began. Over approximately 40 minutes, Luna 3 exposed 29 photographs. Together they covered about 70 percent of the Moon's far side. Taking the pictures was only the first challenge. There were no digital cameras. Luna 3 used photographic film. The spacecraft therefore contained an automated miniature photographic laboratory. After exposure, the film was chemically developed, fixed, dried, and then scanned electronically. The resulting image information could be transmitted toward Earth by radio. It was, in effect, a photographic laboratory and long-distance image transmitter traveling through deep space. Seventeen usable photographs were eventually received on Earth. By modern standards, they were poor. They were grainy. Contrast was limited. Fine surface details were difficult to distinguish. But their scientific importance did not depend upon photographic beauty. For the first time, human beings could see enough of the hidden hemisphere to recognize its large-scale geography. And the far side contained a surprise. It looked different. The familiar Earth-facing hemisphere contains enormous dark regions known as maria—ancient impact basins later flooded by basaltic lava. These broad plains create many of the patterns people have imagined as a “Man in the Moon.” The far side showed far fewer large maria. Instead, much of it appeared bright, rugged, mountainous, and densely cratered. Among the features visible in Luna 3's photographs was a dark region later named Mare Moscoviense—the Sea of Moscow. Other features received names as astronomers began constructing the first maps of the newly revealed hemisphere. Later lunar spacecraft would greatly improve upon Luna 3. Zond probes photographed additional territory. American Lunar Orbiter spacecraft mapped potential Apollo landing regions and other portions of the Moon. Apollo astronauts saw the far side directly as they traveled around the Moon. Modern spacecraft such as the Lunar Reconnaissance Orbiter have mapped the entire lunar surface at resolutions Luna 3's engineers could scarcely have imagined. Those later observations revealed one of the solar system's largest impact structures—the enormous South Pole-Aitken basin—spanning much of the lunar far side. Scientists also came to understand why the two hemispheres differ so strongly. The Moon's crust is generally thicker on the far side. On the near side, enormous ancient impacts penetrated more deeply and were followed by extensive volcanic flooding, producing the dark maria visible from Earth. The far side experienced a different geological history. But before scientists could explain that difference, they first had to discover it. Luna 3 provided the first glimpse. The achievement becomes even more remarkable when placed in chronological perspective. Only two years and three days earlier, Sputnik 1 had become the world's first artificial satellite. Now a spacecraft had traveled to the Moon, passed behind it, automatically photographed an unseen world, developed the pictures onboard, and begun the process of returning those images across hundreds of thousands of kilometers of space. The Space Age was barely two years old. Already, humanity had seen beyond the horizon of another world. Why It Matters: Luna 3's photographs gave humanity its first view of the Moon's far side and revealed that the two lunar hemispheres are strikingly different. The mission transformed an entire hemisphere from an unknowable region into a place that could be photographed, mapped, named, and scientifically investigated. It also demonstrated sophisticated deep-space navigation, automatic photography, onboard film processing, and long-distance image transmission at the very beginning of the Space Age.

 

Also on This Day

2008 — Asteroid 2008 TC3 Strikes Earth Exactly Where Astronomers Predicted

Atmospheric entry approximately 02:46 UTC

Before dawn on October 7, 2008, a small asteroid entered Earth's atmosphere over northern Sudan. Such events are not unusual. Small objects from space enter the atmosphere regularly, most burning up harmlessly before reaching the ground. This event was different. Astronomers knew it was coming. For the first time, an asteroid had been discovered in space before an Earth impact and its arrival time and location successfully predicted. The story began only about 20 hours earlier. At 06:39 UTC on October 6, astronomer Richard Kowalski, working with the Catalina Sky Survey's 1.5-meter telescope on Mount Lemmon in Arizona, detected a rapidly moving object. The observations were sent to the Minor Planet Center. Orbital calculations quickly produced an extraordinary conclusion. The object was on a collision course with Earth. It received the designation 2008 TC3. The asteroid was tiny by planetary-defense standards—only a few meters across. It posed no serious threat to people on the ground. But scientifically, it presented an unprecedented opportunity. Observatories around the world began tracking it. During the hours before impact, professional and amateur astronomers supplied hundreds of positional measurements, allowing scientists to refine the asteroid's trajectory. NASA's Jet Propulsion Laboratory calculated that it would enter Earth's atmosphere above northern Sudan at approximately 02:46 UTC on October 7. And it did. The asteroid struck the atmosphere at roughly 12.8 kilometers per second. At high altitude above the Nubian Desert, it exploded in a brilliant fireball. For a time, scientists thought the object might have been completely destroyed. Then came another remarkable development. Meteor astronomer Peter Jenniskens joined Muawia Shaddad of the University of Khartoum and Sudanese students and researchers to search the predicted fall area. They found meteorites. Eventually, hundreds of fragments were recovered from the Nubian Desert. The meteorites became known collectively as Almahata Sitta, Arabic for “Station Six,” after a nearby railway stop. Scientists could now do something unprecedented. They had astronomical observations of an asteroid while it was still in space. They also possessed physical pieces of that same asteroid in laboratories on Earth. The connection between asteroid astronomy and meteorite science had become direct. Analysis revealed that 2008 TC3 was compositionally unusual, containing a diverse mixture of materials associated with a rare meteorite type known as ureilites. The event also demonstrated the rapidly improving capabilities of near-Earth-object surveys. A small asteroid had been found only hours before impact, yet the international astronomical community had been able to determine where and when it would arrive. Larger hazardous asteroids are generally detectable at much greater distances, potentially providing far more warning. Why It Matters: 2008 TC3 was the first asteroid discovered and tracked in space before its impact with Earth was successfully predicted. The subsequent recovery of meteorites linked telescopic observations of a specific asteroid directly with laboratory samples, while the accurate impact forecast demonstrated an important capability for modern planetary defense.

 

The Bigger Picture

October 7 brings together two events separated by nearly half a century. At first they seem unrelated. Luna 3 looked outward toward the Moon. Astronomers tracking 2008 TC3 looked for something coming toward Earth. But both events depended upon the same fundamental ability: predict where an object in space is going to be. Luna 3 could photograph the far side only because engineers understood its trajectory well enough to send it around the Moon and place it in the correct position at the correct time. 2008 TC3 could be predicted to strike northern Sudan because astronomers measured its position repeatedly and calculated its future path. This is celestial mechanics transformed into practical capability. For centuries, astronomers used mathematics to predict where planets would appear in the sky. During the Space Age, those same principles acquired new purposes. They allowed us to send spacecraft toward other worlds. And increasingly, they allow us to identify objects that might come toward ours. The two events also represent different forms of discovery. Luna 3 discovered by seeing something for the first time. 2008 TC3 demonstrated discovery through prediction. Scientists did not merely watch the asteroid appear as a fireball and then reconstruct what had happened. They saw it coming. That distinction is fundamental to planetary defense. Finding an asteroid after it passes Earth tells us about the population of near-Earth objects. Finding one before an encounter gives us options. For an object only a few meters across, as 2008 TC3 was, the appropriate response is observation. For a substantially larger asteroid discovered sufficiently far in advance, the possibilities could eventually include deflection. That is the same planetary-defense story we encountered on September 26 with DART. DART demonstrated that humanity can deliberately change the motion of an asteroid. 2008 TC3 demonstrated another essential part of the equation: first, we must find it and determine where it is going. October 7 therefore spans two very different frontiers. In 1959, an entire hemisphere of the Moon lay beyond human sight. In 2008, astronomers detected a tiny object in the darkness of space and predicted where it would meet Earth. One expanded the world we could see. The other expanded our ability to anticipate what might reach us. Both began by looking carefully into the sky.

At a Glance

1959 — 03:30 UTC — Luna 3 begins photographing the Moon's far side from roughly 63,500 kilometers above the lunar surface, giving humanity its first views of a hemisphere that had never before been seen.

2008 — Approximately 02:46 UTC — Asteroid 2008 TC3 enters Earth's atmosphere over northern Sudan at the location and time astronomers had predicted, becoming the first asteroid discovered before impact whose collision with Earth was successfully forecast.

October 6

A Planet Around Another Sun

1995 — Astronomers Announce the Discovery of 51 Pegasi b

Time not applicable

On October 6, 1995, two Swiss astronomers announced a discovery that changed humanity's understanding of planetary systems. Michel Mayor and Didier Queloz had detected a planet orbiting 51 Pegasi, an ordinary Sun-like star approximately 50 light-years from Earth. The planet became known as 51 Pegasi b. It was the first planet discovered orbiting a main-sequence star similar to the Sun. Astronomers had wondered about planets around other stars for centuries. Were the planets of our solar system unusual? Or did other stars have worlds of their own? Claims of extrasolar planets had appeared before, but many collapsed under further observation. By the early 1990s, astronomers had discovered planets orbiting a pulsar—the dense remnant of an exploded star—but no planet had yet been reliably detected around an ordinary Sun-like star. Mayor and Queloz were searching for such worlds at the Observatoire de Haute-Provence in southern France. They were not trying to photograph planets directly. Instead, they measured the motion of stars. A planet does not simply orbit a motionless star. Both planet and star orbit their common center of mass. Because a star is vastly more massive, its motion is small. But sufficiently precise spectroscopy can detect the star moving slightly toward and away from Earth. As the star approaches, features in its spectrum shift slightly toward shorter, bluer wavelengths. As it recedes, they shift toward longer, redder wavelengths. This is the radial-velocity method. Mayor and Queloz used an advanced spectrograph called ELODIE to measure those tiny changes. The observations of 51 Pegasi revealed a regular pattern. The star was wobbling. And the wobble repeated approximately every 4.23 days. The most convincing explanation was a planet. But the inferred planet was astonishing. 51 Pegasi b had at least roughly half the mass of Jupiter, yet it orbited its star at only about one-twentieth the Earth-Sun distance. A year on the planet lasted just over four Earth days. Nothing like it existed in our solar system. Mercury, our innermost planet, requires 88 days to orbit the Sun. Jupiter takes nearly twelve years. Planet-formation models of the period generally expected giant planets to form far from their stars, where temperatures were low enough for abundant solid material and ices to contribute to the formation of massive planetary cores. Yet here appeared to be a Jupiter-like planet almost touching its star by comparison. The discovery initially seemed so surprising that skepticism was understandable. But independent observations soon confirmed the signal. A new category of planet entered the astronomical vocabulary: the hot Jupiter. The discovery also forced astronomers to reconsider how planetary systems form and evolve. Perhaps giant planets could form farther from their stars and then migrate inward, their orbits altered through interactions with the disks of gas and dust surrounding young stars or through later gravitational interactions with other planets. If planetary systems could change dramatically after formation, then our own solar system represented only one possible architecture among many. The importance of the discovery extended much farther than one strange planet. Once astronomers knew that planets around ordinary stars could be detected, searches accelerated. New instruments achieved greater precision. Transit surveys watched for the tiny dimming produced when planets crossed in front of their stars. Space telescopes such as Kepler discovered thousands of planetary candidates. Other observatories studied planetary atmospheres. Astronomers found super-Earths, mini-Neptunes, hot Jupiters, compact multiplanet systems, circumbinary planets orbiting two stars, and worlds occupying environments unlike anything represented in our solar system. The question gradually changed. Astronomers no longer asked simply: Do other stars have planets? They began asking: What kinds of planets exist, how do planetary systems form, and how common are worlds that might support life? In 2019, the Nobel Prize in Physics recognized Mayor and Queloz for the discovery of an exoplanet orbiting a solar-type star. 51 Pegasi b was later given the official name Dimidium. The planet itself is unlikely to resemble anything habitable. Its importance lies elsewhere. It revealed that the galaxy contains planetary systems that nature assembled in ways astronomers had scarcely imagined.

Why It Matters: The discovery of 51 Pegasi b opened the modern era of exoplanet astronomy. It provided the first confirmed planet around a Sun-like main-sequence star, challenged existing ideas about planetary formation, and helped transform the search for other worlds from speculation into one of astronomy's most productive fields.

 

Also on This Day

1959 — Luna 3 Sweeps Past the Moon

Closest-approach time not established

Two days after its October 4 launch, the Soviet spacecraft Luna 3 reached the Moon on October 6, 1959. Its journey had a purpose no previous spacecraft had accomplished. Luna 3 was preparing to show humanity a part of the Moon that no human being had ever seen. Because the Moon rotates once in approximately the same time it takes to orbit Earth, nearly the same lunar hemisphere always faces us. The opposite hemisphere—the lunar far side—remained largely hidden. Luna 3's trajectory carried it past the Moon's southern polar region at an altitude of approximately 7,900 kilometers, then around behind the Moon. The flyby itself was crucial. The spacecraft's looping trajectory would place it in the correct geometry to photograph the far side after closest approach. The historic photography occurred the following day, October 7. From tens of thousands of kilometers away, Luna 3 exposed 29 photographs of the previously unseen hemisphere. The spacecraft then developed the photographic film automatically, scanned the images, and transmitted them toward Earth by radio. The pictures were crude. But for the first time, humanity could see the Moon as a complete world rather than only as the familiar face presented to Earth. The images revealed a major geological surprise. The far side contained far fewer of the broad dark volcanic plains—the maria—that dominate much of the near side. Later lunar missions would map that hemisphere with vastly greater precision. But those explorations began with Luna 3's passage around the Moon on October 6.

Why It Matters: Luna 3's October 6 flyby positioned the spacecraft for humanity's first photography of the Moon's far side the following day. The mission turned a permanently hidden hemisphere from an astronomical unknown into an observable landscape.

1990 — Ulysses Launches to Explore the Sun from a New Direction

11:47:16 UTC

On October 6, 1990, Space Shuttle Discovery lifted off from Kennedy Space Center carrying five astronauts and an unusual spacecraft named Ulysses. Its destination was the Sun. But Ulysses would not travel directly toward it. Instead, it would first go to Jupiter. At 11:47:16 UTC, Discovery began mission STS-41. The crew consisted of commander Richard Richards, pilot Robert Cabana, and mission specialists William Shepherd, Bruce Melnick, and Thomas Akers. The principal payload in Discovery's cargo bay was a joint mission of the European Space Agency and NASA. Scientists understood that most planetary exploration took place near a broad plane surrounding the Sun called the ecliptic. Earth and the major planets orbit relatively close to this plane. Consequently, spacecraft launched from Earth naturally begin their journeys within it. That created a problem for solar science. Scientists wanted to study the environment over the Sun's north and south poles. No rocket available could simply launch Ulysses directly into the steeply inclined solar orbit required. Mission designers found a more elegant solution. They would use Jupiter's gravity. About six hours after Discovery reached orbit, the crew deployed Ulysses from the Shuttle's payload bay. A powerful combination of upper stages then accelerated the spacecraft away from Earth. At the time, Ulysses departed Earth faster than any previous human-made spacecraft. It traveled outward across the solar system rather than inward toward the Sun. In February 1992, Ulysses reached Jupiter. The spacecraft passed the giant planet, and Jupiter's gravity dramatically bent its trajectory. Instead of continuing near the ecliptic, Ulysses was thrown into an orbit carrying it far above and below the plane in which the planets travel. The solar poles had become accessible. Ulysses made its first passage over the Sun's southern polar region in 1994 and its first northern polar passage in 1995. The spacecraft did not photograph the Sun in the way a conventional telescope might. Instead, its instruments sampled the solar wind, magnetic fields, energetic particles, cosmic rays, interstellar dust, and other components of the heliosphere. For the first time, scientists could examine the Sun's environment in three dimensions rather than primarily from near the ecliptic plane. Ulysses discovered that the solar wind emerging from high solar latitudes behaved differently from the slower, more variable wind found nearer the solar equator. It investigated how the Sun's magnetic field changes during the solar cycle. It studied cosmic rays entering the heliosphere. And by accident, it made an extraordinary cometary discovery. In 1996, Ulysses unexpectedly encountered the ion tail of Comet Hyakutake, even though the spacecraft was hundreds of millions of kilometers from the comet's nucleus. The encounter revealed that cometary tails could extend much farther through space than previously appreciated. Ulysses had originally been designed for a mission lasting about five years. Instead, it operated for more than 18 years, completing nearly three circuits of the Sun. Operations finally ended in 2009.

Why It Matters: Ulysses was the first mission to investigate the space environment above and below the Sun's poles. By using Jupiter's gravity to leave the ecliptic plane, it gave scientists their first broad three-dimensional survey of the heliosphere and demonstrated once again how celestial mechanics can make possible journeys that rocket power alone cannot easily accomplish.

 

The Bigger Picture

October 6 asks us to reconsider something that seems familiar. The Moon is familiar. The Sun is familiar. Other stars are familiar. But familiarity can conceal how incomplete our knowledge really is. For almost all of human history, people could see only one general hemisphere of the Moon. Luna 3 changed that. Astronomers had observed the Sun for centuries, and spacecraft had been studying it since the beginning of the Space Age. But nearly all those observations were made from close to the plane in which Earth and the other planets orbit. Ulysses changed the perspective. Then came 51 Pegasi b. The planets of our solar system had provided humanity's only detailed example of how a planetary system was organized. There were small rocky planets close to the Sun. Giant planets lived farther away. That arrangement seemed natural. Then astronomers found a giant planet racing around its star every four days. Once again, nature was telling us: the view from where we happen to stand is not the whole story. This is one of astronomy's most persistent lessons. We see the universe from one location. Earth. We inhabit one planetary system. The solar system. We orbit one ordinary star. The Sun. From that limited sample, it is remarkably easy to assume that what surrounds us is typical. Exploration repeatedly breaks that assumption. Travel behind the Moon, and its two hemispheres look surprisingly different. Leave the ecliptic, and the Sun's environment looks different from above its poles. Examine other stars closely enough, and planetary systems appear whose architecture would once have seemed almost impossible. October 6 therefore represents one of the deepest purposes of astronomy and space exploration: change the point of view, and the universe changes with it.

At a Glance

1959 — Closest-approach time not established — Luna 3 passes approximately 7,900 kilometers above the Moon's southern polar region and swings behind the Moon, positioning itself to photograph the lunar far side the following day.

1990 — 11:47:16 UTC — Space Shuttle Discovery launches on STS-41 carrying Ulysses, the ESA-NASA spacecraft that will use Jupiter's gravity to become the first mission to explore the space environment above and below the Sun's poles.

1995 — Time not applicable — Michel Mayor and Didier Queloz announce the discovery of 51 Pegasi b, the first confirmed planet found orbiting a Sun-like main-sequence star.

 

October 5

A More Diverse View from Space

1984 — Challenger Launches a Mission of Firsts

11:03:00 UTC

Fifteen minutes before sunrise on October 5, 1984, Space Shuttle Challenger lifted from Kennedy Space Center carrying a crew unlike any that had flown before. There were seven people aboard—at the time, the largest crew ever launched together on a single spacecraft. Two were women. One was Canadian. One was an oceanographer whose principal laboratory for the next eight days would be the view through Challenger's windows. At 11:03:00 UTC, mission STS-41G began. The crew was commanded by veteran astronaut Robert Crippen, making his fourth journey into space. Jon McBride served as pilot. The three mission specialists were David Leestma, Sally Ride, and Kathryn Sullivan. Ride was already historic. In June 1983 she had become the first American woman in space. Now, for the first time, two women would fly together on the same space mission. The crew also included two payload specialists. Paul Scully-Power, an Australian-born American oceanographer, would concentrate much of his work on observing Earth's oceans from orbit. And Marc Garneau represented Canada. When Challenger reached space, Garneau became the first Canadian to travel beyond Earth. His presence also symbolized Canada's increasingly important role in the Space Shuttle program. Canadian engineering had already produced one of the Shuttle's most recognizable pieces of equipment—the Remote Manipulator System, better known as the Canadarm. STS-41G was therefore international in a way that foreshadowed the increasingly multinational character of human spaceflight. But the mission's principal subject was not the people aboard Challenger. It was the planet below them. STS-41G carried an extensive collection of instruments for observing Earth's atmosphere, oceans, land surfaces, and energy balance. Among the most important payloads was the Earth Radiation Budget Satellite—ERBS. Understanding Earth's climate requires understanding energy. Sunlight delivers energy to the planet. Some is reflected back into space by clouds, ice, land, and oceans. Some is absorbed by Earth's surface and atmosphere and later radiated outward as infrared energy. The balance between incoming and outgoing energy is fundamental to Earth's climate. ERBS was designed to measure that balance. Shortly after reaching orbit, Sally Ride used Challenger's Canadarm to lift the satellite from the payload bay. A problem appeared almost immediately. ERBS's solar arrays did not deploy properly. Mission Control suspected that the hinges had become too cold. Ride oriented the satellite toward the Sun and gently moved it with the robotic arm. The arrays opened. ERBS was released and eventually maneuvered into its operational orbit. Designed for a mission of roughly two years, it continued collecting data for more than two decades, contributing to the long-term study of Earth's radiation balance and climate. Challenger itself carried additional Earth-observation instruments. Radar examined portions of Earth's surface. Cameras recorded landscapes and atmospheric phenomena. Scully-Power concentrated on ocean structures visible from orbit—eddies, currents, waves, and other patterns that could reveal processes difficult to appreciate from ships or aircraft. The human eye itself had become a scientific instrument. Another historic moment came later in the mission. On October 11, Kathryn Sullivan and David Leestma left Challenger's cabin for an extravehicular activity lasting about three and a half hours. Sullivan thereby became the first American woman to walk in space. Their principal task was not ceremonial. They demonstrated equipment for transferring fluids in orbit—technology relevant to the possibility of refueling spacecraft and satellites in space. STS-41G therefore combined several different kinds of progress. It advanced Earth science. It tested technology. It expanded international participation. And its crew visibly broadened the group of people participating directly in human spaceflight. After more than eight days and 132 completed orbits, Challenger returned to Kennedy Space Center on October 13. It was only the second Shuttle mission to land there.

Why It Matters: STS-41G brought together several important developments in human spaceflight. It carried the first two women to fly together in space, made Marc Garneau the first Canadian in space, and later enabled Kathryn Sullivan to become the first American woman to perform a spacewalk. Just as importantly, the mission demonstrated the growing value of spaceflight for studying Earth itself, deploying a satellite and operating instruments that helped scientists investigate the planet's atmosphere, oceans, surface, and energy balance.

 

Also on This Day

1967 — Astronaut Clifton Williams Dies in a Training Accident

Time not established

On October 5, 1967, NASA astronaut and Marine Corps Major Clifton C. “C.C.” Williams Jr. died when the T-38 jet he was flying crashed near Tallahassee, Florida. He was 35 years old. Williams had joined NASA's third group of astronauts in 1963. Like many members of the early astronaut corps, he was an accomplished military test pilot. He had graduated from the U.S. Naval Test Pilot School and accumulated approximately 2,500 hours of flying time, most of it in jet aircraft. At NASA, Williams served as backup pilot for Gemini 10 and worked on launch operations and crew safety. He was also part of the developing Apollo program. Williams had been assigned to the backup crew for an early Apollo mission and was expected to remain within the rotation that could eventually lead to a lunar flight. On October 5, he was flying from Florida toward Houston in a NASA T-38. A mechanical failure led to a loss of control. Williams ejected, but he was traveling too fast and was too low for the escape to save him. His death came during an already painful year for the American space program. Only months earlier, on January 27, astronauts Gus Grissom, Ed White, and Roger Chaffee had died in the Apollo 1 fire during a launch-pad test. Williams became another astronaut lost before he could fly in space. His place in the astronaut rotation was taken by Alan Bean. Bean later served as lunar module pilot of Apollo 12 and became the fourth human being to walk on the Moon. Williams was not forgotten by the crew. Apollo 12 commander Pete Conrad, who had served with Williams on the Gemini 10 backup crew, arranged for Williams's naval aviator wings to travel to the Moon. The insignia was left on the lunar surface in November 1969. Williams's name also appears on the Space Mirror Memorial at Kennedy Space Center, which honors astronauts who died while serving the American space program.

Why It Matters: Clifton Williams's death reminds us that the risks of human spaceflight extend beyond launches and missions. The astronaut corps depended upon constant aircraft training, testing, simulation, and preparation, all of which carried dangers of their own. Williams never reached space, but he was part of the generation whose work and sacrifice helped prepare the way for Apollo.

 

The Bigger Picture

October 5 is fundamentally about who participates in exploration—and what exploration is for. Clifton Williams belonged to the early astronaut corps, an organization drawn largely from a narrow population of American military test pilots. There were reasons for that. Early spacecraft were experimental vehicles, and test pilots possessed precisely the combination of engineering knowledge, flying skill, physical conditioning, and experience with dangerous machinery that NASA needed. But human spaceflight did not remain within that original model. STS-41G makes the change visible. Sally Ride was a physicist. Kathryn Sullivan was a geologist. Paul Scully-Power was an oceanographer. Marc Garneau was a Canadian engineer and naval officer. The Shuttle was becoming not merely a spacecraft piloted by astronauts but a working platform capable of carrying scientists, engineers, international partners, and specialists whose expertise lay outside traditional test piloting. That transition mattered because the purpose of going into space was changing as well. STS-41G spent much of its time looking down. The crew observed oceans. Radar mapped land. Instruments studied the atmosphere. ERBS measured the flow of energy into and out of the Earth system. This is one of the great recurring themes of the Space Age. Humanity went into space partly because we wanted to explore what lies beyond Earth. But once we arrived there, we discovered a remarkable new place from which to understand Earth itself. Weather satellites changed forecasting. Earth-observation spacecraft transformed geology, agriculture, oceanography, mapping, disaster response, and environmental science. Long-term measurements from orbit became essential to understanding climate. The view outward and the view homeward became complementary parts of the same enterprise. There is also a human progression visible between 1967 and 1984. Williams trained during an era when only a handful of nations had sent people into space. Seventeen years later, Challenger carried the first Canadian astronaut. Two women traveled together aboard the same spacecraft. A scientist specializing in Earth's oceans could look directly at those oceans from orbit. Exploration was becoming broader—not only in where humanity could go, but in who could participate and what questions they could ask once they arrived.

At a Glance

1967 — Time not established — NASA astronaut Clifton C. Williams Jr. dies in a T-38 training accident near Tallahassee, Florida; his place in the Apollo crew rotation will later be filled by future Moonwalker Alan Bean.

1984 — 11:03:00 UTC — Space Shuttle Challenger launches on STS-41G with a record seven-person crew, including Sally Ride and Kathryn Sullivan—the first two women to fly together in space—and Marc Garneau, the first Canadian in space.

October 4

The Space Age Begins

1957 — Sputnik 1 Becomes the World's First Artificial Satellite

19:28:34 UTC

On October 4, 1957, a rocket rose from a launch site in the Soviet republic of Kazakhstan carrying a polished metal sphere only 58 centimeters—about 23 inches—across. At 19:28:34 UTC, the Soviet Union launched Sputnik 1, the world's first artificial satellite. Humanity had entered the Space Age. Sputnik itself was remarkably simple. The pressurized aluminum sphere weighed approximately 83.6 kilograms, or 184 pounds. Four long antennas extended behind it, and two radio transmitters broadcast alternating signals at frequencies of approximately 20 and 40 megahertz. Those transmissions produced the feature for which Sputnik became famous: its repeated “beep-beep-beep” radio signal. The sound was technologically simple but historically extraordinary. For the first time, a human-made object was circling Earth and announcing its presence by radio. Sputnik entered an elliptical orbit and completed a circuit of Earth approximately every 96–98 minutes. Anyone with suitable radio equipment could listen. Professional tracking stations heard it. Amateur radio operators heard it. People around the world heard recordings broadcast over radio and television. The signal made something abstract suddenly tangible. Spaceflight was no longer a theoretical possibility. It was happening overhead. The satellite itself also contributed scientific information. The behavior of its radio signals helped researchers study the propagation of radio waves through Earth's ionosphere, while changes in Sputnik's orbit provided information about the density of the upper atmosphere. But Sputnik's greatest effects occurred on Earth. The Soviet Union had demonstrated not only that it could build a satellite but that it possessed a rocket powerful enough to place a substantial object into orbit. That had immediate military implications. A rocket capable of launching a satellite suggested technologies related to those required for an intercontinental ballistic missile. The achievement shocked the United States. American scientists and engineers had also been developing satellite programs for the International Geophysical Year, but none had yet reached orbit. Suddenly, the Soviet Union was first. The psychological impact became known as the “Sputnik crisis.” American political leaders, educators, scientists, and military officials began asking how the Soviet Union had achieved such an important technological first. The response affected education, research, defense, and government organization. Federal support increased for science, mathematics, engineering, and foreign-language education. The Advanced Research Projects Agency—later DARPA—was established in 1958. Most importantly for the history we have been following, Congress passed the National Aeronautics and Space Act, which President Dwight D. Eisenhower signed on July 29, 1958. On October 1, 1958—as we noted only three days ago in this chronology—NASA began operations. Sputnik therefore helped create the circumstances that produced the American civilian space agency. Meanwhile, the satellite continued circling Earth. Its batteries lasted about three weeks. After that, the famous radio signal stopped. But Sputnik itself remained in orbit. Atmospheric drag gradually lowered its trajectory until, on January 4, 1958, after approximately three months and some 1,400 orbits of Earth, Sputnik reentered the atmosphere and burned up. The spacecraft was gone. The age it began was not.

Why It Matters: Sputnik 1 was the first artificial satellite of Earth and is widely regarded as the beginning of the Space Age. Its launch demonstrated that orbital spaceflight was possible, transformed Cold War competition, accelerated investment in science and technology, helped spur the creation of NASA, and began the transition from looking at space to physically entering it.

 

Also on This Day

1959 — Luna 3 Begins Its Journey to the Far Side of the Moon

00:43:40 UTC

Exactly two years after Sputnik 1, the Soviet Union launched another spacecraft from Kazakhstan. Its destination was the Moon. At 00:43:40 UTC on October 4, 1959, Luna 3 began a mission that would reveal something no human being had ever seen: the far side of the Moon. The reason that hemisphere remained hidden was not that the Moon does not rotate. It does. But the Moon rotates once on its axis in approximately the same time it takes to orbit Earth. This synchronous rotation causes nearly the same lunar hemisphere always to face our planet. Small effects called libration allow observers on Earth to glimpse somewhat more than half the lunar surface over time. But a substantial portion remained permanently beyond terrestrial view. For all of human history, people had looked at the Moon without knowing what much of its opposite hemisphere looked like. Luna 3 was designed to change that. The spacecraft weighed approximately 278.5 kilograms and carried the Yenisey-2 photographic television system, along with instruments for studying radiation, charged particles, and micrometeoroids. Its trajectory carried it beyond the Moon and around the lunar far side. On October 6, Luna 3 passed the Moon's southern polar region. Then, on October 7, with the far side illuminated by sunlight, its camera began taking photographs. Over approximately 40 minutes, the spacecraft exposed 29 photographs, covering roughly 70 percent of the previously unseen hemisphere. That alone was an extraordinary achievement. But there was another problem. The photographs were inside a spacecraft hundreds of thousands of kilometers away. Digital imaging did not yet exist. Luna 3 used actual photographic film. The spacecraft therefore carried equipment that automatically developed the film aboard the spacecraft. The resulting images were then scanned electronically and transmitted toward Earth by radio, in a process somewhat analogous to sending a fax across interplanetary space. Seventeen usable images were eventually received. They were poor by modern standards—grainy, noisy, and lacking fine detail. But what they showed was astonishing. The lunar far side looked different from the familiar hemisphere facing Earth. The near side is dominated by broad dark plains called maria, created by ancient volcanic flows that filled enormous impact basins. The far side contained far fewer large maria and appeared more heavily cratered and mountainous. Among the features identified from Luna 3's photographs were Mare Moscoviense, the Sea of Moscow, and the feature initially called Mare Desiderii, the Sea of Dreams. Later spacecraft would photograph the far side in vastly greater detail.

But Luna 3 had done something more fundamental. It had turned an unknown hemisphere into a place humans could see and map. Why It Matters: Luna 3 provided humanity's first photographs of the Moon's far side, revealing that it differed dramatically from the familiar Earth-facing hemisphere. The mission demonstrated sophisticated deep-space navigation, automated photography, onboard film processing, and long-distance image transmission only two years after the beginning of the Space Age.

2004 — SpaceShipOne Wins the Ansari X Prize

Spacecraft release and powered flight began approximately 14:49 UTC

On October 4, 2004—47 years to the day after Sputnik 1—pilot Brian Binnie climbed aboard the small experimental spacecraft SpaceShipOne above California's Mojave Desert. The goal was not orbit. The goal was to demonstrate that a privately developed, reusable crewed spacecraft could reach space twice within two weeks. The challenge had been established by the Ansari X Prize, a $10 million competition intended to encourage development of private human spaceflight. To win, a privately financed vehicle had to reach an altitude of at least 100 kilometers, the internationally recognized Kármán-line boundary commonly used to define the beginning of space, while carrying the equivalent mass of three people. Then it had to do it again within two weeks using the same spacecraft. SpaceShipOne had already completed the first qualifying flight. On September 29, pilot Mike Melvill had flown it to an altitude of approximately 102 kilometers. Five days later came the second attempt. SpaceShipOne did not launch vertically from the ground. Instead, a carrier aircraft called White Knight carried it to an altitude of more than 13 kilometers. At approximately 14:49 UTC, SpaceShipOne separated. Binnie ignited its hybrid rocket motor and accelerated steeply upward. The spacecraft continued climbing after the engine shut down. It reached an altitude of approximately 112 kilometers—nearly 70 miles above Earth. That was comfortably beyond the 100-kilometer requirement. It also exceeded the altitude record for a winged rocket-powered aircraft established by the X-15 four decades earlier. During reentry, SpaceShipOne employed one of its most distinctive innovations. The rear portion of its wings rotated upward into a high-drag “feathered” configuration. Rather than requiring the pilot to maintain a precisely controlled attitude throughout the most difficult portion of reentry, the feathered configuration helped the spacecraft align itself aerodynamically. Once it descended into denser atmosphere, the wings returned to their normal position. SpaceShipOne became a glider. Binnie landed safely back at Mojave. The two qualifying flights had occurred only five days apart. The team had won the $10 million Ansari X Prize. SpaceShipOne did not enter orbit, and it did not immediately produce routine passenger travel into space. Its historical significance was more specific. A privately developed reusable spacecraft had demonstrated repeated crewed suborbital spaceflight without being operated as a government space program. The Smithsonian later placed SpaceShipOne in the National Air and Space Museum alongside such milestones as the Wright Flyer, Charles Lindbergh's Spirit of St. Louis, John Glenn's Friendship 7, and the Bell X-1.

Why It Matters: SpaceShipOne's October 4 flight completed the requirements for the Ansari X Prize and demonstrated that a privately developed reusable crewed spacecraft could make repeated trips beyond the 100-kilometer boundary of space. It became an important milestone in the emergence of commercial human spaceflight.

 

The Bigger Picture

Few dates illustrate the transformation of spaceflight as clearly as October 4. In 1957, Sputnik 1 demonstrated that humanity could place an object into orbit. In 1959, Luna 3 demonstrated that a spacecraft could travel hundreds of thousands of kilometers from Earth, pass behind another world, photograph territory no human had ever seen, process those photographs automatically, and send them home. In 2004, SpaceShipOne demonstrated something different: human spaceflight was beginning to extend beyond the exclusive operation of national governments. The progression is remarkable. Reach space → orbit Earth → explore another world → broaden who can build and operate spacecraft. There is also a striking contrast between Sputnik 1 and Luna 3. Only two years separated them. Sputnik was a radio transmitter inside a metal sphere. Luna 3 was a deep-space robotic observatory equipped to navigate around the Moon, orient itself, photograph an unseen landscape, chemically develop film automatically, scan the results, and transmit the pictures across hundreds of thousands of kilometers. That rapid progression reminds us how quickly the early Space Age developed. The first satellite did not lead to decades of cautious experimentation before humanity ventured farther. Within a year, spacecraft were being aimed toward the Moon. Within two years, one had reached the lunar surface and another had traveled behind it. Within four years, a human being would orbit Earth. And within twelve years of Sputnik, people would walk on the Moon. October 4 also reminds us that anniversaries can influence history. Luna 3 was launched on the second anniversary of Sputnik. SpaceShipOne's prize-winning flight occurred on the 47th anniversary. The United Nations later designated October 4–10 as World Space Week, beginning with the anniversary of Sputnik and ending with the anniversary of the 1967 Outer Space Treaty entering into force. The date therefore became more than the anniversary of one satellite. It became a marker for humanity's entrance into a new realm. Before October 4, 1957, every object ever made by human hands remained on Earth—or returned quickly to it. After that night, there was something else overhead: an object built on Earth, traveling around the world on its own celestial path. The sky had ceased to be only something humanity observed. It had become somewhere humanity could go.

At a Glance

1957 — 19:28:34 UTC — The Soviet Union launches Sputnik 1, the world's first artificial satellite, beginning the Space Age.

1959 — 00:43:40 UTC — Luna 3 launches toward the Moon; three days later it will obtain humanity's first photographs of the lunar far side.

2004 — Approximately 14:49 UTC — Brian Binnie begins SpaceShipOne's second qualifying X Prize spaceflight, reaching approximately 112 kilometers and securing the Ansari X Prize for repeated privately developed crewed suborbital spaceflight.

October 3

The Rocket That Changed the Future

1942 — The A-4 Rocket Makes Its First Successful Flight

Launch time not established

On October 3, 1942, a rocket rose from the German Army research center at Peenemünde on the Baltic coast. Known during development as the A-4, it would later become infamous under another name: V-2. The test vehicle climbed to an altitude of roughly 85–90 kilometers and traveled approximately 190 kilometers before falling back to Earth. It was the first successful flight of a machine unlike anything that had preceded it. The A-4 was a large, long-range, liquid-fueled ballistic rocket. Its engine burned alcohol and liquid oxygen and produced approximately 25 metric tons of thrust. An advanced guidance system controlled the vehicle during powered flight. Previous experimental rockets had demonstrated many of the principles involved. The American physicist Robert Goddard had successfully flown the world's first liquid-fueled rocket in 1926 and subsequently developed increasingly sophisticated rockets incorporating gyroscopic stabilization, pumps, and other technologies. German experimenters had also pursued liquid-fueled rocketry during the 1920s and 1930s. But the A-4 represented a dramatic increase in scale. The October 3 flight demonstrated that a large liquid-fueled rocket could climb to extreme altitude, follow a guided ballistic trajectory, and travel hundreds of kilometers. In purely technological terms, it was a milestone on the road toward spaceflight. But it was not built to explore space. It was built to carry an explosive warhead. Germany was at war, and the A-4 became the V-2, short for Vergeltungswaffe 2—“Vengeance Weapon 2.” Beginning in 1944, V-2 missiles were launched against London, Antwerp, and other targets. Unlike aircraft or earlier weapons, the V-2 descended toward its target at supersonic speed. No warning system could provide meaningful time to intercept it. Thousands of civilians and military personnel were killed or injured by V-2 attacks. Yet even that terrible toll does not encompass the weapon's human cost. Mass production was centered at the underground Mittelwerk factory, where prisoners from the Mittelbau-Dora concentration-camp system were subjected to forced labor under appalling conditions. Thousands died from starvation, disease, exhaustion, beatings, executions, and other abuse. More people died producing the V-2 than were killed by its operational use as a weapon. That history is inseparable from the rocket. After Germany's defeat in 1945, both the United States and Soviet Union sought German rocket hardware, documents, and specialists. The United States brought Wernher von Braun and more than one hundred other German rocket specialists to America through the program eventually known as Operation Paperclip. Captured V-2 rockets were transported to the United States and launched from White Sands, New Mexico, carrying scientific instruments into the upper atmosphere. The Soviet Union similarly obtained German hardware, facilities, documentation, and specialists. Soviet engineers studied and reproduced the technology before developing increasingly capable rockets of their own. The descendants of those programs eventually moved beyond weapons. In the United States, von Braun's team helped develop the Redstone, Jupiter, and Saturn rockets. The Saturn V carried astronauts to the Moon. In the Soviet Union, engineers under Sergei Korolev developed a different technological lineage culminating in the R-7, the rocket family that launched Sputnik and Yuri Gagarin and whose descendants continue to fly. The October 3, 1942, flight therefore occupies an uncomfortable but unavoidable place in space history. The rocket demonstrated technologies that would eventually help humanity reach beyond Earth. But it was created for war, under a dictatorship responsible for enormous crimes, and its later production depended upon murderous exploitation. Both truths belong in the story.

Why It Matters: The successful A-4 flight demonstrated technologies fundamental to later large liquid-fueled rockets and strongly influenced postwar rocket development in both the United States and Soviet Union. But its significance cannot be separated from its origin as a Nazi weapon and from the concentration-camp prisoners who suffered and died producing it. The history of spaceflight contains extraordinary achievements, but understanding that history also requires remembering the human costs embedded within some of its technological foundations.

 

Also on This Day

1962 — Wally Schirra Flies Sigma 7 Six Times Around Earth

Launch: 12:15:12 UTC

On October 3, 1962, astronaut Walter “Wally” Schirra climbed into the small Mercury spacecraft he had named Sigma 7. The name reflected the kind of mission he intended to fly. The Greek letter sigma is used in mathematics to represent summation. For Schirra, Sigma 7 represented the sum of the engineering work that had gone into Mercury—and the seven astronauts originally chosen for the program. At 12:15:12 UTC, an Atlas rocket lifted Sigma 7 from Cape Canaveral. Schirra became the fifth American in space and the third American to orbit Earth. John Glenn and Scott Carpenter had each completed three orbits earlier that year. Schirra would attempt six. The mission, officially designated Mercury-Atlas 8, emphasized engineering and spacecraft operations. One of its most important questions concerned resources. Mercury carried limited electrical power and maneuvering fuel. If future missions were to remain in space longer, astronauts would have to demonstrate that those resources could be conserved. Schirra deliberately allowed Sigma 7 to drift for extended periods rather than continuously controlling its attitude. The technique greatly reduced fuel consumption. He also conducted spacecraft tests, photographed Earth, made visual observations, and experimented with using stars for orientation. At one point Schirra transmitted a television message from orbit, one of the early live broadcasts from an American spacecraft. After six circuits of Earth, he prepared for reentry. His landing demonstrated another aspect of the mission's precision. Sigma 7 splashed down in the Pacific after 9 hours, 13 minutes, and 11 seconds in flight. The spacecraft landed only a few miles from the recovery carrier USS Kearsarge. It was the first crewed American orbital mission to end with a Pacific Ocean splashdown. Schirra later described Sigma 7 as a “textbook flight.” The characterization was appropriate. Mercury was becoming less about proving that an American could survive orbit and more about demonstrating that people and spacecraft could operate there predictably and efficiently. Schirra would later become the only astronaut to fly in all three of America's pioneering human-spaceflight programs: Mercury, Gemini, and Apollo.

Why It Matters: Sigma 7 demonstrated disciplined spacecraft operation, fuel conservation, and precise reentry during America's longest orbital mission to that point. Mercury was evolving from an experiment in human survival into the foundation for the more complex operations required by Gemini and Apollo.

1985 — Atlantis Makes Its First Flight

15:15:30 UTC

On October 3, 1985, another spacecraft began a much longer career. At 15:15:30 UTC, Space Shuttle Atlantis lifted off from Kennedy Space Center on mission STS-51J. It was Atlantis's first journey into space. Atlantis was the fourth operational orbiter constructed for NASA's Space Shuttle fleet, following Columbia, Challenger, and Discovery. Its first mission was unusual because much of what it carried and accomplished was classified. STS-51J was a dedicated mission for the United States Department of Defense. Commander Karol Bobko led a five-person crew consisting of pilot Ronald Grabe and mission specialists David Hilmers, Robert Stewart, and William Pailes. The mission's primary payload involved military communications satellites. Because of the classified nature of the flight, NASA's normal public coverage stopped shortly after Atlantis reached orbit. After four days in space, Atlantis landed at Edwards Air Force Base in California on October 7. Its first mission was complete. But the orbiter's career was only beginning. Atlantis would eventually become one of the most important vehicles in the Shuttle fleet. It launched the Magellan spacecraft toward Venus in 1989. Later that year, it launched Galileo toward Jupiter. In 1991, Atlantis carried the Compton Gamma Ray Observatory, one of NASA's Great Observatories, into orbit. During the 1990s, Atlantis became closely associated with the Shuttle-Mir program, completing multiple dockings with the Russian space station and helping build experience in international long-duration operations. It later played a major role in assembling and servicing the International Space Station. And on July 8, 2011, Atlantis lifted off on STS-135, the final mission of the entire Space Shuttle program. The spacecraft that began its career with a classified military mission on October 3, 1985, therefore ended it almost 26 years later by closing one of the most recognizable chapters in the history of human spaceflight.

Why It Matters: STS-51J began the 33-mission career of Space Shuttle Atlantis. Over the following quarter century, the orbiter would launch major planetary and astronomical spacecraft, help pioneer cooperation with Mir, support construction of the International Space Station, and ultimately fly the final mission of the Space Shuttle era.

 

The Bigger Picture

October 3 offers an unusually concentrated view of the evolution of the rocket. In 1942, the A-4 demonstrated that a large liquid-fueled rocket could travel to extraordinary altitude and range. Twenty years later, an Atlas rocket carried Wally Schirra into orbit. Twenty-three years after that, Atlantis climbed toward space using a combination of reusable liquid-fueled engines and enormous solid rocket boosters. Technologically, it is tempting to draw a simple line: A-4 → ballistic missiles → launch vehicles → human spaceflight → reusable spacecraft. There is truth in that progression. But it is incomplete. Technology does not carry its own moral purpose. A rocket engine can accelerate a warhead toward a city. A related technology can carry a scientific instrument above Earth's atmosphere. Another can place a human being into orbit. Still another can launch a probe toward Jupiter. The physical laws are the same. The purposes are not. That distinction is particularly important on October 3. The people who suffered and died in the V-2 program should not disappear from the history simply because technologies developed there later contributed to space exploration. Nor should the history imply that modern spaceflight emerged from one nation or one group alone. Robert Goddard's pioneering experiments in the United States, Konstantin Tsiolkovsky's theoretical work in Russia, Hermann Oberth's writings and experiments in Europe, Soviet engineering under Sergei Korolev, American research, and contributions from thousands of engineers and scientists across many countries all belong to the much larger story. By the time Schirra flew Sigma 7, the rocket had become a means of placing a human being into orbit. By the time Atlantis flew, rockets had become part of a transportation system capable of carrying people, satellites, observatories, and planetary spacecraft. October 3 therefore gives us something more complicated than a story of technological progress. It asks us to remember that the history of exploration contains both achievement and responsibility. Understanding how we reached space means remembering both.

At a Glance

1942 — Launch time not established — The A-4 makes its first successful test flight from Peenemünde, demonstrating large-scale liquid-fueled ballistic-rocket technology that will strongly influence postwar missile and space-launch development.

1962 — 12:15:12 UTC — Wally Schirra launches aboard Sigma 7 on Mercury-Atlas 8, completing six Earth orbits during a 9-hour, 13-minute engineering mission.

1985 — 15:15:30 UTC — Space Shuttle Atlantis launches on STS-51J for its maiden flight, beginning a 33-mission career that will continue through the final Space Shuttle mission in 2011.