Hubble Captures a "Five-Star" Rated Gravitational Lens
NASA's Hubble Space Telescope has captured the first-ever picture of a group of five star-like images of a single distant quasar.
The multiple-image effect seen in the Hubble picture is produced by a process called gravitational lensing, in which the gravitational field of a massive object - in this case, a cluster of galaxies - bends and amplifies light from an object - in this case, a quasar - farther behind it. (More at Hubble Site)
This is a unique view of the disk galaxy NGC 5866 tilted nearly edge-on to our line-of-sight. Hubble's sharp vision reveals a crisp dust lane dividing the galaxy into two halves. The image highlights the galaxy's structure: a subtle, reddish bulge surrounding a bright nucleus, a blue disk of stars running parallel to the dust lane, and a transparent outer halo. NGC 5866 is a disk galaxy of type "S0" (pronounced s-zero). Viewed face on, it would look like a smooth, flat disk with little spiral structure. It remains in the spiral category because of the flatness of the main disk of stars as opposed to the more spherically rotund (or ellipsoidal) class of galaxies called "ellipticals." Such S0 galaxies, with disks like spirals and large bulges like ellipticals, are called 'lenticular' galaxies. NGC 5866 lies in the Northern constellation Draco, at a distance of 44 million light-years. It has a diameter of roughly 60,000 light-years only two-thirds the diameter of the Milky Way, although its mass is similar to our galaxy. This Hubble image of NGC 5866 is a combination of blue, green and red observations taken with the Advanced Camera for Surveys in February 2006. (More at Hubble Site)
Staring into the crowded, dusty core of two merging galaxies, NASA's Hubble Space Telescope has uncovered a region where star formation has gone wild.
The interacting galaxies appear as a single, odd-looking galaxy called Arp 220. The galaxy is a nearby example of the aftermath of two colliding galaxies. In fact, Arp 220 is the brightest of the three galactic mergers closest to Earth. This latest view of the galaxy is yielding new insights into the early universe, when galactic wrecks were more common. The sharp eye of Hubble's Advanced Camera for Surveys has unveiled more than 200 mammoth star clusters. The clusters are the bluish-white dots scattered throughout the image. (More at Hubble Site)
Dark Energy Co-Discoverer Adam Riess Shares Shaw Prize in Astronomy for 2006
Astronomer Adam Riess, of the Space Telescope Science Institute and the Johns Hopkins University, and two colleagues, have been awarded this year's $1 million Shaw Prize in astronomy for their discovery of the mysterious "dark energy" that is causing the universe to expand at an ever-faster rate. (More at Hubble Site)
Pluto's Two Small Moons Officially Named Nix and Hydra
A pair of small moons that NASA's Hubble Space Telescope discovered orbiting Pluto now have official names: Nix and Hydra. Photographed by Hubble in 2005, Nix and Hydra are roughly 5,000 times fainter than Pluto and are about two to three times farther from Pluto than its large moon, Charon, which was discovered in 1978. (More at Hubble Site)
Hubble Reveals Two Dust Disks Around Nearby Star Beta Pictoris
Detailed images of the nearby star Beta Pictoris, taken by NASA's Hubble Space Telescope, confirm the existence of not one but two dust disks encircling the star. The images offer tantalizing new evidence for at least one Jupiter-size planet orbiting Beta Pictoris.
The finding ends a decade of scientific speculation that an odd warp in the young star's debris disk may actually be another inclined disk. The recent Hubble Advanced Camera for Surveys view - the best visible-light image of Beta Pictoris - clearly shows a distinct secondary disk that is tilted by about 4 degrees from the main disk. The secondary disk is visible out to roughly 24 billion miles from the star, and probably extends even farther, said astronomers. This Hubble image of Beta Pictoris clearly shows a primary dust disk and a much fainter secondary dust disk. Astronomers used the Advanced Camera's coronagraph to block out the light from the bright star. (More at Hubble Site)
Hubble's Advanced Camera for Surveys Resumes Exploring the Universe
After a brief hiatus, the Advanced Camera for Surveys aboard NASA's Hubble Space Telescope is back in business, probing the far reaches of space in a quest to understand the true nature of the universe's most dominant constituent: dark energy.
This is one of the first images of the universe taken after the ACS camera resumed science operation on July 4th. The camera was offline for nearly two weeks as NASA engineers switched to a backup power supply after the camera's primary power supply failed. (More at Hubble Site)
NASA's Hubble Space Telescope has captured an image of a cosmic explosion that is quite similar to fireworks on Earth. In the nearby galaxy, the Small Magellanic Cloud, a massive star has exploded as a supernova, and begun to dissipate its interior into a spectacular display of colorful filaments. The greenish-blue supernova remnant, E0102, resides 50 light-years away from the edge of a bright glowing massive star-forming region. (More at Hubble Site)
Hubble Identifies Stellar Companion to Distant Planet
NASA's Hubble Space Telescope has for the first time identified the parent star of a distant planet (system name OGLE-2003-BLG-235L/MOA-2003-BLG-53L) discovered in 2003 through ground-based gravitational microlensing. Gravitational microlensing occurs when a foreground star amplifies the light of a background star that momentarily aligns with it. Follow-up observations by Hubble in 2005 separated the light of the slightly offset foreground star from the background star. This allowed the host star to be identified as a red dwarf star located 19,000 light-years away. The Hubble observations allow for the planet's mass and the orbit from its parent red star to be determined. In this artist's concept, the rings and moon around the gas giant are hypothetical, but plausible, given the nature of the family of gas giant planets in our solar system. (More at Hubble Site)
Astrophysicist Michael G. Hauser (Space Telescope Science Institute deputy director and adjunct professor in the Department of Physics and Astronomy of the Johns Hopkins University in Baltimore, Md.) is a member of the Cosmic Background Explorer (COBE) science team sharing the Peter Gruber Foundation's 2006 Cosmology Prize. The prize's gold medal and $250,000 cash prize was presented to the team on August 15 at the General Assembly of the International Astronomical Union in Prague, Czech Republic. The COBE satellite was launched in 1989 to measure the early universe's diffuse infrared and microwave radiationn. The COBE science team was honored by the foundation for the satellite's multiple accomplishments. (More at Hubble Site)
NASA's Hubble Space Telescope has uncovered what astronomers are reporting as the dimmest stars ever seen in any globular star cluster. Globular clusters are spherical concentrations of hundreds of thousands of stars.
These clusters formed early in the 13.7-billion-year-old universe. The cluster NGC 6397 is one of the closest globular star clusters to Earth. Seeing the whole range of stars in this area will yield insights into the age, origin, and evolution of the cluster. (More at Hubble Site)
Dark matter and normal matter have been wrenched apart by the tremendous collision of two large clusters of galaxies. This composite image shows the galaxy cluster 1E 0657-56, also known as the "bullet cluster." The hot gas detected by Chandra in X-rays is seen as two pink clumps in the image and contains most of the "normal" matter in the two clusters. The bullet-shaped clump on the right is the hot gas from one cluster, which passed through the hot gas from the other larger cluster during the collision. An optical image from Magellan and the Hubble Space Telescope shows the galaxies in orange and white. The blue areas in this image show where astronomers find most of the mass in the clusters.
This active region of star formation in the Large Magellanic Cloud (LMC), as photographed by NASA's Hubble Space Telescope, unveils wispy clouds of hydrogen and oxygen that swirl and mix with dust on a canvas of astronomical size. The LMC is a satellite galaxy of the Milky Way.
This particular region within the LMC, referred to as N 180B, contains some of the brightest known star clusters. This image was taken with Hubble's Wide Field Planetary Camera 2 in 1998 using filters that isolate light emitted by hydrogen and oxygen gas. (More at Hubble Site)
Robert Williams Named President-Elect of the International Astronomical Union
The General Assembly of the International Astronomical Union (IAU), meeting in Prague, Czech Republic, has named Dr. Robert Williams, Space Telescope Science Institute (STScI), as its President-Elect. He will become IAU President in 2009. Dr. Williams served as STScI director from 1993 until 1998. He is the principal investigator for the Hubble Deep Field -- one of humankind's deepest, most detailed visible-light views of the universe.
The IAU is a body of distinguished professional astronomers, founded in 1919 to promote and safeguard the science of astronomy in all its aspects through international cooperation. The IAU named Dr. Catherine Cesarsky of the European Southern Observatory (ESO) as its President and Ian Corbett (ESO) as its Assistant General Secretary for the term 2006-2009. (More at Hubble Site)
Cassiopeia A - The Colorful Aftermath of a Violent Stellar Death
A new image taken with NASA's Hubble Space Telescope provides a detailed look at the tattered remains of a supernova explosion known as Cassiopeia A (Cas A). It is the youngest known remnant from a supernova explosion in the Milky Way. The new Hubble image shows the complex and intricate structure of the star's shattered fragments. The image is a composite made from 18 separate images taken in December 2004 using Hubble's Advanced Camera for Surveys (ACS). (More at Hubble Site)
This NASA Hubble Space Telescope image is a never-before-seen astronomical alignment of a moon traversing the face of Uranus, and its accompanying shadow. The white dot near the center of Uranus' blue-green disk is the icy moon Ariel. The 700-mile-diameter satellite is casting a shadow onto the cloud tops of Uranus. To an observer on Uranus, this would appear as a solar eclipse, where the moon briefly blocks out the Sun as its shadow races across Uranus's cloud tops. Though such "transits" by moons across the disks of their parents are commonplace for some other gas giant planets, such as Jupiter, the satellites of Uranus orbit the planet in such a way that they rarely cast shadows on the planet's surface. Uranus is tilted so that its spin axis lies nearly in its orbital plane. The planet is essentially tipped over on its side. The moons of Uranus orbit the planet above the equator, so their paths align edge-on to the Sun only every 42 years. This color composite image was created from images at three wavelengths in near infrared light obtained with Hubble's Advanced Camera for Surveys on July 26, 2006. (More at Hubble Site)
Planet Or Failed Star? NASA's Hubble Telescope Photographs One of Smallest Stellar Companions Ever Seen
Astronomers using NASA's Hubble Space Telescope have photographed one of the smallest objects ever seen around a normal star beyond our Sun. Weighing in at 12 times the mass of Jupiter, the object is small enough to be a planet. The conundrum is that it's also large enough to be a brown dwarf, a failed star. The Hubble observation of the diminutive companion to the low-mass red dwarf star CHXR 73 is a dramatic reminder that astronomers do not have a consensus in deciding which objects orbiting other stars are truly planets -- even though they have at last agreed on how they will apply the definition of "planet" to objects inside our solar system. (More at Hubble Site)
Tracing the Evolution of the First Galaxies in the Universe
A systematic search for the first bright galaxies to form in the early universe has revealed a dramatic jump in the number of such galaxies around 13 billion years ago. These observations of the earliest stages in the evolution of galaxies provide new evidence for the hierarchical theory of galaxy formation -- the idea that large galaxies built up over time as smaller galaxies collided and merged. Astronomers at the University of California, Santa Cruz, used NASA's Hubble Space Telescope to explore the formation of galaxies during the first 900 million years after the Big Bang. They reported their latest findings in the September 14 issue of the journal Nature. Deep observations in three dark patches of sky -- the Hubble Ultra Deep Field and the Great Observatories Origins Deep Survey fields -- gathered the faint light emitted 13 billion years ago by stars in primeval galaxies. Only the brightest galaxies could be detected at such great distances. The researchers observed hundreds of bright galaxies at around 900 million years after the Big Bang. But when they looked deeper, about 200 million years earlier in time, they only found one. Relaxing their search criteria a bit turned up a few more candidates, so there must have been a lot of merging of smaller galaxies during those 200 million years.
This panel shows four candidate galaxies that are likely to have redshifts of 7 and thus have emitted their light when the universe was just 750 million years old. Astronomers can determine when light was emitted from a distant source by its redshift, a measure of how the expansion of the universe stretched the wavelengths of the light as it traveled through space across vast distances. (More at Hubble Site)
NASA's Hubble Finds Hundreds of Young Galaxies in Early Universe
Astronomers analyzing two of the deepest views of the cosmos made with NASA's Hubble Space Telescope have uncovered a gold mine of galaxies, more than 500 that existed less than a billion years after the Big Bang. This sample represents the most comprehensive compilation of galaxies in the early universe, researchers said. The discovery is scientifically invaluable for understanding the origin of galaxies, considering that just a decade ago early galaxy formation was largely uncharted territory. Astronomers had not seen even one galaxy that existed when the universe was a billion years old, so finding 500 in a Hubble survey is a significant leap forward for cosmologists. This Hubble Space Telescope image shows 28 of the more than 500 young galaxies the researchers uncovered in their analysis of two Hubble surveys. (More at Hubble Site)
April 24 Marks a Triumphant Ten Years in Space for Hubble Space Telescope
In its first ten years, the 12.5-ton Earth-orbiting NASA's Hubble has studied 13,670 objects, has made 271,000 individual observations, and has returned 3.5 terabytes of data, which have been archived as a scientific treasure trove for future generations of astronomers. Its rapid-fire scientific achievements have resulted in over 2,651 scientific papers. Hubble's photographic hall of fame includes the deepest view ever of the Universe in visible light; a peek into the environs of supermassive galactic black holes; the majestic birth of stars in monstrous stellar clouds; planetary systems forming around other stars; extraordinary arcs, shells, and ribbons of glowing gas sculpted by the deaths of ordinary stars; mega-megaton blasts produced by the impact of a comet into the cloud tops of Jupiter; the surface of mysterious Pluto; and galaxies at the edge of space and time. (More at Hubble Site)
