Space Hubble Telescope News

Life Is Too Fast, Too Furious for This Runaway Galaxy

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Our spiral-shaped Milky Way galaxy lives in a comparatively quiet backwater region of the universe. This is not the case for galaxies crammed together inside huge clusters. As they zip around within a cluster, gas can be pulled from their disks due to a process called ram pressure stripping. Galaxy ESO 137-001 is one example. The star-city looks like it is "leaking" as it plunges through the Norma galaxy cluster.

(More at HubbleSite.com)
 
Hubble Witnesses an Asteroid Mysteriously Disintegrating

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Though fragile comet nuclei have been seen falling apart as they near the Sun, nothing like the slow breakup of an asteroid has ever before been observed in the asteroid belt. A series of Hubble Space Telescope images shows that the fragments are drifting away from each other at a leisurely one mile per hour. This makes it unlikely that the asteroid is disintegrating because of a collision with another asteroid. A plausible explanation is that the asteroid is crumbling due to a subtle effect of sunlight. This causes the rotation rate to slowly increase until centrifugal force pulls the asteroid apart. The asteroid's remnant debris, weighing in at 200,000 tons, will in the future provide a rich source of meteoroids.

(More at HubbleSite.com)
 
New iBooks Textbook Helps Visually Impaired Visit the Stars Through Touch and Sound

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Children with visual disabilities can experience striking deep-space images in a free, multi-touch iBooks textbook for the iPad entitled "Reach for the Stars: Touch, Look, Listen, Learn." Astronomers at the Space Telescope Science Institute have teamed up with the SAS Corporation, the National Braille Press, and the National Federation of the Blind to create a book to inspire students of all abilities. Students with visual impairments can access the book using the VoiceOver screen reader that is available on every iPad. The book is available as a free download from Apple's iBooks Store at https://itunes.apple.com/us/book/reach-for-stars-touch-look/id763516126?mt=11.

(More at HubbleSite.com)
 
Dr. Roeland van der Marel Appointed as STScI Lead on Proposed "Wide View" Space Telescope

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The Space Telescope Science Institute (STScI) in Baltimore, Maryland, has appointed Dr. Roeland van der Marel to lead its work on a proposed NASA space telescope that will provide images as sharp as the Hubble Space Telescope, but over a hundred times larger area. The space observatory, called the Wide-Field Infrared Survey Telescope-Astrophysics Focused Telescope Assets (WFIRST-AFTA), is being studied for launch in the mid-2020s, pending program approval by NASA. The telescope will be used to probe the distribution of dark matter and the characteristics of dark energy, measure the abundance and characteristics of planets orbiting other stars, and will provide observations and surveys to study many other astrophysical subjects. STScI is presently the science operations center for the Hubble Space Telescope and the science and mission operations center for the James Webb Space Telescope, scheduled for launch in 2018. Van der Marel joined the STScI staff in 1997. He is also an adjunct professor in the Department of Physics and Astronomy at the Johns Hopkins University in Baltimore, Maryland. He is an expert on black holes and the structure of galaxies.

(More at HubbleSite.com)
 
Hubble Video Shows Shock Collision Inside Black Hole Jet

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One of the trademarks of the Star Wars film episodes is the dreaded Death Star battle station that fires a beam of directed energy powerful enough to blow up planets. The real universe has such fireworks, and they are vastly more powerful than the Star Wars creation. These extragalactic jets are tearing across hundreds of light-years of space at 98 percent the speed of light. Instead of a battle station, the source of the killer beam is a supermassive black hole weighing many million or even a billion times the mass of our sun. Energy from the spinning black hole, and its titanic magnetic fields, shape a narrow jet of gas blasting out a galaxy's center. Hubble has been used over the past 25 years to photograph and rephotograph a jet blasting out the heart of the elliptical galaxy 3C 264 (also known as NGC 3862). Hubble's sharp vision reveals that the jet has a string-of-pearls structure of glowing knots of material. When these images were assembled into a time-lapse movie, they reveal – to the surprise of astronomers – a faster-moving bright knot rear-ending the bright knot in front of it. The resulting shock collision further accelerates particles that produce a focused beam of deadly radiation. The jet is moving so fast toward us it gives the illusion that it is traveling faster than the speed of light. But not to worry, the host galaxy is 260 million light-years away. We are seeing the jet as it looked before the dinosaurs appeared on Earth, and our planet was suffering a global mass extinction.

(More at HubbleSite.com)
 
Telescopes Team Up to Find Distant Uranus-Sized Planet Through Microlensing

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The majority of planets discovered outside our solar system orbit close to their parent stars because these planets are the easiest to find. But to fully understand how distant planetary systems are put together, astronomers must conduct a census of all the planets around a star. So they need to look farther away from the star-from about the distance of Jupiter is from our sun, and beyond.

Now, astronomers using NASA's Hubble Space Telescope and the W. M. Keck Observatory in Hawaii have confirmed the existence of a Uranus-sized exoplanet orbiting far from its central star, discovered through a technique called gravitational microlensing. Microlensing occurs when a foreground star magnifies the light of a background star that momentarily aligns with it. The unique signature of the event, which is influenced by the relative motion of the stars across space, can reveal clues to the nature of the foreground star and any associated planets. Gravitational microlensing can find cold planets in long-period orbits that other methods cannot detect. This finding opens a new piece of discovery space in the extrasolar planet hunt: to uncover planets as far from their central stars as Jupiter and Saturn are from our sun.

(More at HubbleSite.com)
 
Hubble Zooms in on Shrapnel from an Exploded Star

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Not long before the dawn of recorded human history, our distant ancestors would have witnessed what appeared to be a bright new star briefly blazing in the northern sky, rivaling the glow of our moon. In fact, it was the titanic detonation of a bloated star much more massive than our sun. Now, thousands of years later, the expanding remnant of that blast can be seen as the Cygnus Loop, a donut-shaped nebula that is six times the apparent diameter of the full moon. The Hubble Space Telescope was used to zoom into a small portion of that remnant, called the Veil Nebula. Hubble resolves tangled rope-like filaments of glowing gases. Supernovae enrich space with heavier elements used in the formation of future stars and planets – and possibly life.

Learn even more about the Veil Nebula in a discussion with Hubble Heritage Team scientists during the live Hubble Hangout at 3pm EDT on Thurs., Sept. 24 at New Hubble 25th Anniversary Image Released .

(More at HubbleSite.com)
 
NASA Introduces New, Wider Set of Eyes on the Universe: Baltimore's Space Telescope Science Institute to Partner on New NASA 'Wide-View' Space Telescope

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After years of preparatory studies, NASA is formally starting an astrophysics mission designed to help unlock the secrets of the universe the Wide-Field Infrared Survey Telescope (WFIRST). WFIRST will image large regions of the sky in near-infrared light to answer fundamental questions about dark energy and the structure and evolution of the universe. It will also find and characterize planets beyond our solar system, and as a general-purpose observatory, revolutionize many other astrophysical topics. WFIRST will have a mirror the same size as Hubble's, but it will have a 100 times wider view of space. Slated for launch in the mid-2020s, it will complement the capabilities of NASA's other major astrophysical observatories.

WFIRST is managed at NASA's Goddard Space Flight Center in Greenbelt, Maryland, with participation by the Jet Propulsion Laboratory (JPL) in Pasadena, California; the Space Telescope Science Institute (STScI) in Baltimore, Maryland; the Infrared Processing and Analysis Center (IPAC), also in Pasadena; and a science team comprised of members from U.S. research institutions across the country. STScI will be a partner on the WFIRST science operations and will focus during the mission formulation phase on the observation scheduling system, wide-field imaging data processing system, and the data archive.

To learn more about the WFIRST mission and STScI, join a live Hubble Hangout discussion with scientists at 3:00 p.m. EST on Thurs., Feb. 18, at WFIRST: Uncovering Cosmic Mysteries | Hubble Hangout.

(More at HubbleSite.com)
 
Hubble Catches Views of a Jet Rotating with Comet 252P/LINEAR

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For thousands of years, humans have recorded sightings of mysterious comets sweeping across the nighttime skies. These celestial wanderers, "snowballs" of dust and ice, are swift-moving visitors from the cold depths of space. Some of them periodically visit the inner solar system during their journeys around the sun.

Astronomers using NASA's Hubble Space Telescope captured images of Comet 252P/LINEAR just after it swept by Earth on March 21. The visit was one of the closest encounters between a comet and our planet. The comet traveled within 3.3 million miles of Earth, or about 14 times the distance between our planet and the moon. The images reveal a narrow, well-defined jet of dust ejected by the comet's icy, fragile nucleus. The jet also appears to change direction in the images, which is evidence that the comets nucleus is spinning. The spinning nucleus makes the jet appear to rotate like the water jet from a rotating lawn sprinkler. These observations also represent the closest celestial object Hubble has observed, other than the moon. The comet will return to the inner solar system again in 2021.

(More at HubbleSite.com)
 
Hubble Spots Possible Water Plumes Erupting on Jupiter's Moon Europa

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New findings from NASA's Hubble Space Telescope show suspected water plumes erupting from Jupiter's icy moon Europa. These observations bolster earlier Hubble work suggesting that Europa is venting water vapor. A team of astronomers, led by William Sparks of the Space Telescope Science Institute in Baltimore, Maryland, observed these finger-like projections while viewing Europa's limb as the moon passed in front of Jupiter. The team was inspired to use this observing method by studies of atmospheres of planets orbiting other stars.

The plumes are estimated to rise about 125 miles before, presumably, raining material back down onto Europa's surface. This is exciting because Europa is a plausible place for life to have developed beyond the Earth. If the venting plumes originate in a subsurface ocean, they could act as an elevator to bring deep-sea life above Europa's surface, where it could be sampled by visiting spacecraft. This offers a convenient way to access the chemistry of that ocean without drilling through miles of ice. To view NASA's Europa plumes summary video, visit the YouTube link at
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(More at HubbleSite.com)
 
The Dawn of a New Era for Supernova 1987A

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In February 1987, on a mountaintop in Chile, telescope operator Oscar Duhalde stood outside the observatory at Las Campanas and looked up at the clear night sky. There, in a hazy-looking patch of brightness in the sky — the Large Magellanic Cloud (LMC), a neighboring galaxy - was a bright star he hadn't noticed before.

That same night, Canadian astronomer Ian Shelton was at Las Campanas observing stars in the Large Magellanic Cloud. As Shelton was studying a photographic plate of the LMC later that night, he noticed a bright object that he initially thought was a defect in the plate. When he showed the plate to other astronomers at the observatory, he realized the object was the light from a supernova. Duhalde announced that he saw the object too in the night sky. The object turned out to be Supernova 1987A, the closest exploding star observed in 400 years. Shelton had to notify the astronomical community of his discovery. There was no Internet in 1987, so the astronomer scrambled down the mountain to the nearest town and sent a message to the International Astronomical Union's Bureau for Astronomical Telegrams, a clearing house for announcing astronomical discoveries.

Since that finding, an armada of telescopes, including the Hubble Space Telescope, has studied the supernova. Hubble wasn't even in space when SN 1987A was found. The supernova, however, was one of the first objects Hubble observed after its launch in 1990. Hubble has continued to monitor the exploded star for nearly 30 years, yielding insight into the messy aftermath of a star's violent self-destruction. Hubble has given astronomers a ring-side seat to watch the brightening of a ring around the dead star as the supernova blast wave slammed into it.

(More at HubbleSite.com)
 
Comet or Asteroid? Hubble Discovers that a Unique Object is a Binary

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Astronomers categorize the minor bodies in the solar system according to their location and physical composition. Comets are a loose collection of ice and dust that fall in toward the Sun from beyond the orbits of the major planets, and grow long tails of dust and gas along the way. Asteroids are rocky or metallic and are relegated to a zone between Mars and Jupiter. But nature isn't that tidy. The Hubble Space Telescope photographed a pair of asteroids orbiting each other that have a tail of dust, which is definitely a comet-like feature. The odd object, called 2006 VW139/288P, is the first known binary asteroid that is also classified as a main-belt comet. Roughly 5,000 years ago, 2006 VW139/288P probably broke into two pieces due to a fast rotation.

(More at HubbleSite.com)
 
Hubble's Celestial Snow Globe

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It's beginning to look a lot like the holiday season in this NASA Hubble Space Telescope image of a blizzard of stars, which resembles a swirling snowstorm in a snow globe. The stars are residents of the globular star cluster Messier 79, or M79, located 41,000 light-years from Earth, in the constellation Lepus. The cluster is also known as NGC 1904.

(More at HubbleSite.com)
 
Hubble Reveals a Giant Cosmic "Bat Shadow"

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Like a fly that wanders into a flashlight’s beam, a young star’s planet-forming disk is casting a giant shadow, nicknamed the “Bat Shadow.” Hubble’s near-infrared vision captured the shadow of the disk of this fledgling star, which resides nearly 1,300 light-years away in a stellar nursery called the Serpens Nebula. In this Hubble image, the shadow spans approximately 200 times the length of our solar system. It is visible in the upper right portion of the picture. The young star and its disk likely resemble what the solar system looked like when it was only 1 or 2 million years old.

(More at HubbleSite.com)
 
Hubble Views the Star that Changed the Universe

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Though the universe is filled with billions upon billions of stars, NASA's Hubble Space Telescope has been trained on a single variable star that in 1923 altered the course of modern astronomy. And, at least one famous astronomer of the time lamented that the discovery had shattered his world view. The star goes by the inauspicious name of Hubble variable number one, or V1, and resides two million light-years away in the outer regions of the neighboring Andromeda galaxy, or M31. V1 is a special class of pulsating star called a Cepheid variable that can be used to make reliable measurements of large cosmic distances. The star helped Edwin Hubble show that Andromeda lies beyond our galaxy. Prior to the discovery of V1 many astronomers, including Harlow Shapley, thought spiral nebulae, such as Andromeda, were part of our Milky Way galaxy. Others weren't so sure. In fact, Shapley and Heber Curtis held a public debate in 1920 over the nature of these nebulae. But it took Edwin Hubble's discovery just a few years later to settle the debate. Hubble sent a letter, along with a light curve of V1, to Shapley telling him of his discovery. After reading the note, Shapley reportedly told a colleague, "here is the letter that destroyed my universe." The universe became a much bigger place after Edwin Hubble's discovery.

In commemoration of this landmark observation, astronomers with the Space Telescope Science Institute's Hubble Heritage Project partnered with the American Association of Variable Star Observers (AAVSO) to study the star. AAVSO observers followed V1 for six months, producing a plot, or light curve, of the rhythmic rise and fall of the star's light. Based on this data, the Hubble Heritage team scheduled Hubble telescope time to capture Wide Field Camera 3 images of the star at its dimmest and brightest light levels. The observations are being presented on May 23 at the meeting of the American Astronomical Society in Boston, Mass. Copies of the photograph Edwin Hubble made in 1923 flew onboard space shuttle Discovery in 1990 on the mission that deployed Hubble. Two of the remaining five copies were part of space shuttle Atlantis's cargo in 2009 for NASA's fifth servicing mission to Hubble. Edwin Hubble's observations of V1 became the critical first step in uncovering a larger, grander universe. He went on to measure the distances to many galaxies beyond the Milky Way by finding Cepheid variables within them. The velocities of those galaxies, in turn, allowed him to determine that the universe is expanding. The space telescope that bears his namesake continues using Cepheids to refine the expansion rate of the universe and probe galaxies far beyond Edwin Hubble's reach.

(More at HubbleSite.com)
 
Mars: Closest Encounter

These two images, taken 11 hours apart with NASA's Hubble Space Telescope, reveal two nearly opposite sides of Mars. Hubble snapped these photos as the red planet was making its closest approach to Earth in almost 60,000 years. Mars completed nearly one half a rotation between the two observations.

(More at HubbleSite.com)
 
Celestial Composition

Amid a backdrop of far-off galaxies, the majestic dusty spiral NGC 3370 looms in the foreground in this NASA Hubble Space Telescope image. Recent observations taken with the Advanced Camera for Surveys show intricate spiral arm structure spotted with hot areas of new star formation. But this galaxy is more than just a pretty face. Nearly 10 years earlier, NGC 3370, located in the constellation Leo, hosted a bright exploding star.

(More at HubbleSite.com)
 
Hubble Assists Rosetta Comet Mission

Results from NASA's Hubble Space Telescope played a major role in preparing ESA's ambitious Rosetta mission for its new target, comet 67P/Churyumov-Gerasimenko (67P/C-G). For the first time in history, Rosetta will land a probe on a comet and study its origin. Hubble precisely measured the size, shape, and rotational period of comet 67P/C-G. The Hubble observations revealed comet 67P/C-G to be a football-shaped object of approximately three miles by two miles in size---large enough to provide a landing site for the Rosetta mission probe.

(More at HubbleSite.com)
 
Farthest, Faintest Solar System Objects Found Beyond Neptune

Astronomers using NASA's Hubble Space Telescope have discovered three of the faintest and smallest objects ever detected beyond Neptune. Each object is a lump of ice and rock - roughly the size of Philadelphia - orbiting beyond Neptune and Pluto, where the icy bodies may have dwelled since the formation of the solar system 4.5 billion years ago. They reside in a ring-shaped region called the Kuiper Belt, which houses a swarm of icy rocks that are leftover building blocks, or "planetesimals," from the solar system's creation. The biggest surprise of the Hubble search is that so few small Kuiper Belt members were discovered. With Hubble's exquisite resolution, Bernstein and his co-workers expected to find at least 60 Kuiper Belt members as small as 10 miles (15 km) in diameter - but only three were found. Two snapshots, taken 12 hours apart, were combined to produce this Hubble Space Telescope image of a Kuiper Belt object (named 2000 FV53) moving across the sky. Hubble's Advanced Camera for Surveys tracked the object on Jan. 26, 2003. Like all the planets, this solar-system member appears to move relative to the fixed stars and galaxies in the background. This particular object was discovered from Hawaii in March 2000 and used to help target the Hubble observations.

(More at HubbleSite.com)
 
NASA Approves James Webb Space Telescope Mirror Architecture

NASA today announced a major milestone in the development of the James Webb Space Telescope (JWST), the selection of a beryllium-based mirror technology for the telescope's 6.5-meter primary mirror. The JWST prime contractor, Northrop Grumman, Redondo Beach, Calif., recommended to NASA the mirror technology, supplied by Ball Aerospace & Technologies Corporation, Boulder, Colo., be selected for the JWST primary mirror.

(More at HubbleSite.com)
 
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