HubbleSite

The ancients thought that stars were fixed pinpoints of light on the sky. Today we know that they are all moving, like fish in a pond. This so-called proper motion is so small that it is not noticeable to the human eye over a single lifetime. But Hubble can precisely track stellar motions to razor-sharp precision. Not surprisingly the nearest star to our Sun, Proxima Centauri, is one of the fastest moving across the sky. Hubble astronomers have found that it will pass in front of two far-more distant background stars, once in 2014 and again in 2016. This will afford a very rare opportunity to see how Proxima's gravity warps the image of the background stars by bending their light. This effect, called gravitational lensing, can be used to estimate Proxima Centauri's mass and establish the presence of any planets orbiting the star. View the full article

The distinctive shape of the Ring Nebula, the glowing shroud around a dying Sun-like star, makes it a popular celestial object that appears in many astronomy books. New observations of the Ring Nebula by NASA's Hubble Space Telescope, however, reveal a new twist on an iconic nebula. The Hubble images offer the best view yet of the nebula, revealing a complex structure. The observations have allowed astronomers to construct the most precise three-dimensional model of the glowing gas shroud, called a planetary nebula. Based on the new observations, the Hubble research team suggests that the ring wraps around a blue football-shaped structure that protrudes out of opposite sides of the ring. The nebula is tilted toward Earth so that astronomers see the ring face-on. View the full article

Deep inside the Hyades star cluster, a pair of burned-out stars are yielding clues to the presence of rocky planets that may have whirled around them. Asteroid debris is 'raining' into the hot atmospheres of these white dwarfs. Asteroids should consist of the same material that form terrestrial planets, and seeing evidence of asteroids points to the possibility of Earth-sized planets in the same system. Hubble's Cosmic Origins Spectrograph observed silicon and only low levels of carbon in the white dwarfs' atmospheres. Silicon is a major ingredient of the rocky material that constitutes Earth and other solid planets in our solar system. Astronomers used sophisticated computer models of white dwarf atmospheres to determine the abundances of various elements that can be traced to planets in the Hubble spectrograph data. View the full article

The Space Telescope Science Institute has appointed Dr. Massimo Stiavelli as the James Webb Space Telescope (JWST) Mission Head. Stiavelli will be responsible for the development and operations of the JWST Science and Operations Center at STScI. He has been acting JWST Mission Head since January 2012. The largest space observatory ever developed, JWST is scheduled for launch in 2018. Stiavelli succeeds Dr. Kathy Flanagan, who was appointed the Institute's Deputy Director in October 2012. Stiavelli has worked at the Institute for over 17 years. His many positions at the Institute include instrument scientist for three Hubble cameras. Stiavelli has been working on the JWST project since 1996. View the full article

Comet ISON is potentially the "comet of the century" because around the time the comet makes its closest approach to the Sun, on November 28, it may briefly become brighter than the full Moon. Right now the comet is far below naked-eye visibility, and so Hubble was used to snap the view of the approaching comet, which is presently hurtling toward the Sun at approximately 47,000 miles per hour. When the Hubble picture was taken on April 10, the comet was slightly closer than Jupiter's orbit at a distance of 386 million miles from the Sun. Even at that great distance the Sun is warming the comet enough to trigger outgassing from its frozen gases locked up in the solid nucleus. Hubble photographed a jet blasting dust particles off the sunward-facing side of the comet's nucleus. Preliminary measurements from the Hubble images suggest that the nucleus of ISON is no larger than three or four miles across. The comet was discovered in September 2012 by the Russian-led International Scientific Optical Network (ISON) using a 16-inch telescope. View the full article

Unlike other celestial objects there is no question how the Horsehead Nebula got its name. This iconic silhouette of a horse's head and neck pokes up mysteriously from what look like whitecaps of interstellar foam. The nebula has graced astronomy books ever since its discovery over a century ago. But Hubble's infrared vision shows the horse in a new light. The nebula, shadowy in optical light, appears transparent and ethereal when seen at infrared wavelengths. This pillar of tenuous hydrogen gas laced with dust is resisting being eroded away by the radiation from a nearby star. The nebula is a small part of a vast star-forming complex in the constellation Orion. The Horsehead will disintegrate in about 5 million years. As part of Hubble's 23rd anniversary Horsehead Nebula release, amateur astronomers around the world were invited to send in their Horsehead Nebula photos. Visit the Hubble Heritage Horsehead Image Release to view the contributions via Flickr and Tumblr and to send us your own image. View the full article

NASA and the Space Telescope Science Institute (STScI) have announced the selection of 17 new Hubble Fellows. The Hubble Fellowship Program now includes all research relevant to present and future missions in NASA's Cosmic Origins theme. These missions currently include the Herschel Space Observatory, the Hubble Space Telescope (HST), the James Webb Space Telescope (JWST), the Stratospheric Observatory for Infrared Astronomy (SOFIA), and the Spitzer Space Telescope. STScI in Baltimore, Md., administers the Hubble Fellowship Program for NASA. More than 310 of the most prominent and active scientists in this field have been supported at a crucial phase in their careers by this program, and the Hubble Fellowship Program continues to be one of the highlights of NASA's pursuit of excellence in space science. The new Hubble Fellows will begin their programs in the fall of 2013. View the full article

A long time ago, in a galaxy far, far away, a star detonated with enough energy to briefly shine with an intrinsic brightness of one billion of our suns. The beacon of radiation arrived at Earth 10 billion years later and was captured in a Hubble Space Telescope deep survey of the universe. It is the farthest, and earliest, supernova of its type detected to date. More than simply an example of the ancient fireworks in the young and effervescent universe, the supernova belongs to a special class of stellar detonations that are so reliably bright, they can be used as intergalactic milepost markers. Supernovae like this one provided the first observational evidence that the universe is expanding at an ever-faster rate. Our understanding of the accelerating universe, however, is only as solid as the reliability of supernovae as solid yardsticks for measuring cosmic distances. This record-breaker is so ancient it can be used to test competing theories about how such supernovae exploded in the universe's early days and compare them with nearby supernovae seen today. Its discovery is part of an ongoing program, where different teams of astronomers are using Hubble to push ever farther back into the early epoch of star formation. View the full article

NASA's Chandra X-ray telescope has made the first detection of X-ray emission from young solar-type stars that lie outside our Milky Way galaxy. They live in a region known as the "Wing" of the Small Magellanic Cloud, a satellite galaxy of our Milky Way. X-rays from young stars trace how active their magnetic fields are. Magnetic activity provides clues to a star's rotation rate and the rising and falling of hot gas in the star's interior. Astronomers suggest that if the X-ray properties of young stars are similar in different environments around our galaxy, then other related properties, such as the formation of planets, are also likely to be similar. In this composite image from NASA's Great Observatories of the Wing, the Chandra data are shown in purple; visible light seen by the Hubble Space Telescope is in red, green, and blue; and infrared data from the Spitzer Space Telescope are colored red. View the full article

Looking up through hundreds of colored filters and spectral glasses, 526 people shattered the record for the Largest Astronomy Lesson. Under the Texas night sky, students were instructed on the lawn of the Long Center for the Performing Arts at the South by Southwest (SXSW) festival in Austin on Sunday, March 10, 2013. View the full article

You can't be older than your parents. But there is a nearby star that at first glance looks like it is older than the universe! Hubble Space Telescope astronomers are coming to grips with this paradox by improving the precision of the observations used to estimate the age of this "Methuselah star." Around the year 2000, estimates for the star's age were about 16 billion years. But the universe is about 13.8 billion years old, based on a meticulous calibration of the expansion of space and analysis of the microwave afterglow from the big bang. Hubble data and improved theoretical calculations were used to recalculate the star's age and lower the estimate to 14.5 billion years, within a measurement uncertainty of plus or minus 800 million years. This places the star within a comfortable range to be younger than the universe. Astronomers have to collect a lot of information to deduce a star's age because it doesn't come with a birth certificate. They have to take into account where the star is in its life history, the detailed chemistry of the star, and its intrinsic brightness. Hubble's contribution was to reduce the uncertainty on the star's true distance. With that improved accuracy, the intrinsic brightness of the star is better known. The ancient star is still spry for its age. It is speeding past us at 800,000 miles per hour. Its orbit can be traced back to the halo of our galaxy, which is a "retirement home" for stars that were born long before the Milky Way was even fully assembled. View the full article

The universe is eerie enough without giving us an apparition of a 1980s video game alien attacker. This oddball-looking object is really a mirage created by the gravitational field of a foreground cluster of galaxies warping space and distorting the background images of more distant galaxies. This effect, called gravitational lensing, can make multiple mirror image copies of the light coming from a far-flung galaxy. It is a powerful tool for seeing remote galaxies that otherwise would not be observable by Hubble because they are too dim and far away. In this Hubble photo a background spiral galaxy is warped into an image that resembles a cartoon of a simulated space invader. The foreground massive cluster, called Abell 68, lies 2 billion light-years away. The brightened and stretched lensed images come from galaxies far behind it. View the full article

Peering deep into the vast stellar halo that envelops our Milky Way galaxy, astronomers using NASA's Hubble Space Telescope have uncovered tantalizing evidence for the possible existence of a shell of stars that are a relic of cannibalism by our Milky Way. Hubble was used to precisely measure, for the first time ever, the sideways motions of a small sample of stars located far from the Milky Way galaxy's center. Their unusual lateral motion is circumstantial evidence that the stars may be the remnants of a shredded galaxy that was gravitationally ripped apart by the Milky Way billions of years ago. These stars support the idea that the Milky Way grew, in part, through the accretion of smaller galaxies. View the full article

Everything's bigger in Texas, and a life-sized model of the world's largest space telescope, NASA's James Webb Space Telescope, will be on display at the South by Southwest (SXSW) Interactive Festival along with Webb-related exhibits, educational events, interactives, visualizations, scientists, and much more. The NASA events at SXSW will occur March 8-10, 2013, in Austin. The Webb telescope model is coming to SXSW just in time to highlight the fact that this spring NASA is starting to bring together some of the major parts of the observatory. In 2013, NASA will begin to integrate the four science instruments that will be attached to the telescope. NASA is partnering with Northrop Grumman, the Space Telescope Science Institute, Ball Aerospace, Microsoft Research, and the University of Texas' Astronomy Department to bring an amazing display of science and technology to SXSW. View the full article

A mysterious infant star, swaddled inside a dusty blanket, behaves like a police strobe light. The newly discovered object offers clues into the early stages of star formation, when a lot of gas and dust is being rapidly sucked into a newly forming binary star. Every 25.34 days, the object, designated LRLL 54361, unleashes a burst of light. The flashes may be due to material suddenly being dumped onto the growing protostars, unleashing a blast of radiation each time the stars get close to each other in their orbits. The phenomenon has been seen in later stages of star birth, but never in such a young system, nor with such intensity and regularity. LRLL 54361 was discovered by the Spitzer Space Telescope as a variable object inside the star-forming region IC 348, located 950 light-years away. The Hubble Space Telescope was used to confirm the Spitzer observations and revealed the detailed structure around the protostar. Hubble resolved two cavities that are traced by light scattered off their edges above and below a dusty disk. Astronomers will continue monitoring LRLL 54361 using other telescopes, including the Herschel Space Telescope, and hope to eventually obtain more direct measurements of the binary star and its orbit. View the full article

Working with astronomical image processors at the Space Telescope Science Institute in Baltimore, Md., renowned astrophotographer Robert Gendler has taken science data from the Hubble Space Telescope archive and combined it with his own ground-based observations to assemble a photo illustration of the magnificent spiral galaxy M106. Gendler retrieved archival Hubble images of M106 to assemble a mosaic of the center of the galaxy. He then used his own and fellow astrophotographer Jay GaBany's observations of M106 to combine with the Hubble data in areas where there was less coverage, and finally, to fill in the holes and gaps where no Hubble data existed. View the full article

Jason Kalirai of the Space Telescope Science Institute in Baltimore, Md., has been awarded the 2013 Newton Lacy Pierce Prize. This annual prize from the American Astronomical Society is for outstanding achievement in observational astronomy by an astronomer under the age of 36. Kalirai, 34, received the award for his contributions to the field of stellar and galactic astrophysics. Kalirai has also devised new methods to measure the age of the Milky Way galaxy. View the full article

Newly released Hubble Space Telescope images of a vast debris disk encircling the nearby star Fomalhaut, and of a mysterious planet circling it, may provide forensic evidence of a titanic planetary disruption in the system. Astronomers are surprised to find that the debris belt is wider than previously known, spanning a gulf of space from 14 billion miles to nearly 20 billion miles from the star. Even more surprisingly, the latest Hubble images have allowed a team of astronomers to calculate that the planet follows an unusual elliptical orbit that carries it on a potentially destructive path through the vast dust ring. The planet, called Fomalhaut b, swings as close to its star as 4.6 billion miles, and the outermost point of its orbit is 27 billion miles away from the star. The orbit was re-calculated from the newest Hubble observation made in 2012. The Fomalhaut team led by Paul Kalas (University of California, Berkeley) considers this circumstantial evidence that there may be other planet-like bodies in the system that gravitationally disrupted Fomalhaut b to place it in such a highly eccentric orbit. His team is presenting their finding today at the 221st meeting of the American Astronomical Society in Long Beach, Calif. View the full article

Astronomers using NASA's Hubble and Spitzer space telescopes have probed the stormy atmosphere of a brown dwarf named 2MASSJ22282889-431026, creating the most detailed "weather map" yet for this class of cool, star-like orbs. The forecast shows wind-driven, planet-sized clouds enshrouding these strange worlds. Brown dwarfs form out of condensing gas, as stars do, but lack the mass to fuse atoms and produce energy. Instead, these objects, which some call failed stars, are more similar to gas planets with their complex, varied atmospheres. The new research is a stepping stone toward a better understanding not only brown dwarfs, but also of the atmospheres of planets beyond our solar system. Hubble and Spitzer simultaneously watched the brown dwarf as its light varied in time, brightening and dimming about every 90 minutes as the body rotated. Astronomers found the timing of this change in brightness depended on whether they looked using different wavelengths of infrared light. The variations are the result of different layers or patches of material swirling around in the brown dwarf in windy storms as large as Earth itself. Spitzer and Hubble see different atmospheric layers because certain infrared wavelengths are blocked by vapors of water and methane high up, while other infrared wavelengths emerge from much deeper layers. Daniel Apai, the principal investigator of the research from the University of Arizona, Tucson, presented the results at the American Astronomical Society meeting on January 8 in Long Beach, Calif. A study describing the results, led by Esther Buenzli, also of the University of Arizona, is published in the Astrophysical Journal Letters. View the full article

NASA's Hubble Space Telescope has been providing astounding images of the universe since April 1990 and has led to remarkable discoveries. NASA's James Webb Space Telescope is the next-generation telescope that will peer even deeper into space and unveil even more mysteries. Both of these extraordinary telescopes are now the topics of two free e-books available from the Apple iBookstore. The e-book "Hubble Space Telescope: Discoveries" takes the reader on a tour of some of Hubble's most significant science successes, combined with some of the telescope's technology and history. In the e-book called the "James Webb Space Telescope: Science Guide," readers will learn how the Webb telescope will reveal in much more detail mysteries of the universe that the Hubble is not able to see. View the full article

'Tis the season for holiday decorating and tree-trimming. Not to be left out, astronomers using NASA's Hubble Space Telescope have photographed a festive-looking nearby planetary nebula called NGC 5189. The intricate structure of this bright gaseous nebula resembles a glass-blown holiday ornament with a glowing ribbon entwined. View the full article

Using NASA's Hubble Space Telescope, astronomers have uncovered a previously unseen population of seven primitive galaxies that formed more than 13 billion years ago, when the universe was less than 3 percent of its present age. The deepest images to date from Hubble yield the first statistically robust sample of galaxies that tells how abundant they were close to the era when galaxies first formed. The results show a smooth decline in the number of galaxies with increasing look-back time to about 450 million years after the big bang. The observations support the idea that galaxies assembled continuously over time and also may have provided enough radiation to reheat, or reionize, the universe a few hundred million years after the big bang. These pioneering observations blaze a trail for future exploration of this epoch by NASA's next-generation spacecraft, the James Webb Space Telescope. Looking deeper into the universe also means peering farther back in time. The universe is now 13.7 billion years old. The newly discovered galaxies are seen as they looked 350 million to 600 million years after the big bang. Their light is just arriving at Earth now. The public is invited to participate in a "First Census of Galaxies Near Cosmic Dawn" webinar, in which key astronomers of the Hubble Ultra Deep Field 2012 team will discuss how they obtained their result and what it tells us about galaxy formation in the very early universe. Participants will be able to send in questions for the panel of experts to discuss. The webinar will be broadcast at 1:00 pm EST on Friday, December 14, 2012. View the full article

Bright pink nebulae almost completely encircle a spiral galaxy in this NASA/ESA Hubble Space Telescope image of NGC 922. The ring structure and the galaxy's distorted spiral shape result from a smaller galaxy scoring a cosmic bull's-eye, hitting the center of NGC 922 some 330 million years ago. Hubble's image of NGC 922 consists of a series of exposures taken in visible light with the Wide Field Camera 3, and in visible and near-infrared light with the Wide Field and Planetary Camera 2. View the full article

Now you see it, now you don't. Douglas Clowe of Ohio University in Athens, Ohio, is reporting on new Hubble observations that do not find an unusually dense clump of dark matter in the universe that a different Hubble team reported on earlier this year. The region of interest lies at the center of a collision among massive galaxy clusters in Abell 520, located 2.4 billion light-years away. "The earlier result presented a mystery. But in our observations we didn't see anything surprising in the core," said Clowe. "Our measurements are in complete agreement with how we would expect dark matter to behave." Because dark matter is not visible, its presence and distribution is found indirectly through its gravitational effects. The gravity from both dark and luminous matter warps space, bending and distorting light from galaxies and clusters behind it like a giant magnifying glass. Astronomers can use this effect, called gravitational lensing, to infer the presence of dark matter in massive galaxy clusters. Both teams used this technique to map the dark matter in the merging cluster. Clowe is encouraging other scientists to study the Hubble data and conduct their own analysis on the cluster. View the full article

Spectacular jets powered by the gravitational energy of a supermassive black hole in the core of the elliptical galaxy Hercules A illustrate the combined imaging power of two of astronomy's cutting-edge tools, the Hubble Space Telescope's Wide Field Camera 3, and the recently upgraded Karl G. Jansky Very Large Array (VLA) radio telescope in New Mexico. View the full article