Astronomy and Stars
Discussions about astronomy and stars. As we look further out what can we find in the universe beyond Earth's atmosphere?
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A natural color NASA Hubble Space Telescope view of the full disk of the giant planet Jupiter shows numerous comet Shoemaker-Levy 9 impact sites as seen on July 22, 1994. View the full article
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Ultraviolet image of Jupiter taken by the Wide Field Camera of the Hubble Space Telescope. The image shows Jupiter's atmosphere at a wavelength of 2550 Angstroms after many impacts by fragments of comet Shoemaker-Levy 9. View the full article
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This is a NASA's Hubble Space Telescope image of the impact sites of fragments "D" and "G" from Comet Shoemaker-Levy 9 which collided with the giant planet Jupiter. The picture has been image processed to correct for the curvature of the disk of Jupiter, so that the spot appears flat, as if the viewer were hovering directly overhead. The large feature was created by the impact of comet fragment "G" which impacted Jupiter on July 18, 1994. The smaller feature to the left was created on July 17, by the impact of comet fragment "D". View the full article
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This series of images, which spans more than five days beginning at 5:33 p.m. EDT on July 16, 1994, was obtained with NASA's Hubble Space Telescope's Wide Field Planetary Camera-2 using the methane filter that reveals details in Jupiter's higher atmosphere. These images show the development of the ejecta from site A, formed by the impact of the first fragment of comet P/Shoemaker-Levy 9. View the full article
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Image of Jupiter with NASA's Hubble Space Telescope's Planetary Camera. Eight impact sights are visible. From left to right are the E/F complex (barely visible on the edge of the planet), the star shaped H site, the impact sites for tiny N, Q1, small Q2, and R, and on the far right limb the D/G complex. The D/G complex also shows extended haze at the edge of the planet. The features are rapidly evolving on timescales of days. The smallest features in the this image are less than 200 kilometers across. This image is a color composite of three filters at 9530, 5500, and 4100 Angstroms. View the full article
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This Hubble telescope image of the giant planet Jupiter reveals the impact sites of two fragments from comet Shoemaker-Levy 9. Twenty-one large chunks of the comet rained down upon Jupiter in July 1994. The impact sites, located in the planet's Southern Hemisphere, are the dark spots in the upper left of the photograph. View the full article
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These images of Jupiter, by NASA's Hubble Space Telescope, reveal the impact sites of fragments "D" and "G" from Comet Shoemaker-Levy 9. The upper right corners of each image points north, showing the impact sites located in Jupiter's southern hemisphere at a latitude of 44 degrees. View the full article
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This comparison of visible light (blue) and far-ultraviolet (FUV) images of Jupiter taken with the Wide Field Planetary Camera-2 (WFPC-2) on NASA's Hubble Space Telescope show how the appearance of the planet and of comet Shoemaker-Levy 9 impact sites differ at these two wavelengths (1400-2100 and 3100-3600 Angstroms). The images taken 20 minutes apart on July 17,1994 (around 19:00 UT), show the impact sites on the southern hemisphere, from left to right, of comet fragments C, A, and E, about 12, 23, and 4 hours after each collision. Jupiter's satellite 10 is seen crossing above the center of the disk, and the famous Great Red Spot is near the eastern limb. View th…
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This NASA Hubble Space Telescope image of Jupiter's cloudtops was taken at 5:32 EDT on July 16, 1994, shortly after the impact of the first fragment (A) of comet Shoemaker-Levy 9. A violet (410 nanometer) filter of the Wide Field Planetary Camera 2 was used to make the image 1.5 hours after the impact. View the full article
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Astronomers at the Space Telescope Science Institute huddle around monitors to get a glimpse of images from fragment A of comet P/Shoemaker-Levy 9's collision with Jupiter in July 1994. View the full article
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Sequence of images showing evidence for a plume near the terminator of Jupiter at the time of comet P/Shoemaker-Levy 9's fragment A impact with Jupiter in July 1994. View the full article
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This is a composite photo, assembled from separate images of Jupiter and cornet P/Shoemaker-Levy 9, as imaged by the Wide Field & Planetary Camera 2 (WFPC2), aboard. NASA's Hubble Space Telescope (HST). View the full article
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Astronomers using the Hubble telescope have uncovered the strongest evidence yet that the planet-making process is common in the Milky Way Galaxy. Observations clearly reveal that great disks of dust – the raw material for planet formation – are swirling around at least half and probably many more of the stars in the Orion Nebula, a star-forming region only 1,500 light-years from Earth. View the full article
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Astronomers using the Hubble telescope have found seemingly conclusive evidence for a massive black hole in the center of the giant elliptical galaxy M87, located 50 million light-years from Earth in the constellation Virgo. Earlier observations suggested that the black hole was present, but they were not decisive. This observation provides very strong support for the existence of gravitationally collapsed objects, which were predicted 80 years ago by Albert Einstein's general theory of relativity. This image shows a spiral-shaped disk of hot gas in the core of M87. Hubble measurements indicate that the disk's rapid rotation is strong evidence that it contains a massive…
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The Hubble telescope has returned valuable new images of supernova 1994I in the inner regions of the "Whirlpool Galaxy," M51, located 20 million light-years from Earth in the constellation Canes Venatici. The arrow marks the supernova's location. The supernova was discovered by amateur astronomers on April 2, 1994 and has been the target of investigations by astronomers using ground-based optical and radio telescopes. At its brightest, around April 10, the supernova was about 100 million times more luminous than the Sun. A supernova is a violent stellar explosion that destroys a massive star. View the full article
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The Hubble telescope has obtained the best images yet of a mysterious mirror-imaged pair of rings of glowing gas encircling the site of the stellar explosion called supernova 1987A. One possibility for these "hula hoops" of gas is that the two rings might be caused by a high-energy beam of radiation that is sweeping across the gas, like a searchlight sweeping across clouds. Though all of the rings appear inclined to our view (so that they appear to intersect), they are probably in three different planes. The small, bright ring lies in a plane containing the supernova; one larger ring lies in front of and the other behind the smallest one. View the full article
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This is a composite HST image taken in visible light showing the temporal evolution of the brightest region of comet P/Shoemaker-Levy 9. In this false-color representation, different shades of red color are used to display different intensities of light. View the full article
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This is the clearest view yet of the distant planet Pluto and its moon Charon, as revealed by the Hubble telescope. Hubble snapped this image when the planet was 2.6 billion miles (4.4 billion kilometers) from Earth, or nearly 30 times the separation between Earth and the Sun. The two objects are shown as clearly separate and sharp disks. View the full article
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The giant gaseous planet Jupiter and its moon Io are featured in this Hubble telescope picture. One of Io's many volcanoes, Pele, appears as a dark spot surrounded by an irregular orange oval on the lower part of the moon. The orange material has been ejected from the volcano and spread over a huge area. Though the volcano was first discovered by the Voyager spacecraft, the distinctive orange color of the volcanic deposits is a new discovery. View the full article
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This Hubble telescope image [right] reveals a faint galaxy, the home of a quasar. The wealth of new detail in this picture helps solve a three-decade-old mystery about the true nature of quasars, the most distant and energetic objects in the universe. The picture clearly shows that the quasar, called 1229+204, lies in the core of a galaxy that has a common shape, consisting of two spiral arms of stars connected by a bar-like feature. The host galaxy is in a spectacular collision with a dwarf galaxy. That collision apparently fuels the quasar "engine" at the galaxy's center - presumably a massive black hole - and also triggers many sites of new star-formation. A ground-b…
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The Space Telescope Science Institute (STScI) has recently selected 11 young scientists for the 1994 Hubble Postdoctoral Fellowship Program. The awardees were selected from a pool of applications from highly-qualified candidates worldwide. Inaugurated in 1990, the Hubble Fellowship Program funds research opportunities for a significant fraction of the approximately two hundred Ph.D. astronomers who graduate annually. The program is a joint venture between NASA and STScI in cooperation with astronomical institutions across the United States. View the full article
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Two astronomers have discovered that our own Milky Way galaxy and most of its neighboring galaxies, contained within a huge volume of the universe, one billion light-years in diameter, are drifting with respect to the more distant universe. This startling result may imply that the universe is "lumpier" on a much larger scale than can be readily explained by any current theory. "The new observations thus strongly challenge our understanding of how the universe evolved," says Dr. Tod Lauer of the National Optical Astronomy Observatories (NOAO). View the full article
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These images of Comet P/Shoemaker- Levy 9 (1993e) fragments were made by NASA's Hubble Space Telescope (HST). The cometary chunks are expected to plunge into Jupiter's atmosphere in July 1994. The comet was torn into numerous pieces by the massive planet's gravitational pull as it passed by Jupiter in summer 1992. View the full article
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A NASA Hubble Space Telescope "natural color" image of the material surrounding the star Eta Carinae, as imaged by the Wide Field Planetary Camera 2 (WFPC-2). The Camera was installed in the Hubble Space Telescope during the STS-61 Hubble Servicing Mission. The WFPC-2 optically corrects for the aberration of the telescope's primary minor, restoring the telescope's vision to its originally planned clarity. View the full article
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A NASA Hubble Space Telescope image of a region of the Great Nebula in Orion, as imaged by the Wide Field Planetary Camera 2. This is one of the nearest regions of very recent star formation (300,000 years ago). The nebula is a giant gas cloud illuminated by the brightest of the young hot stars at the top of the picture. Many of the fainter young stars are surrounded by disks of dust and gas, that are slightly more than twice the diameter of the solar system (or 100 Astronomical Units in diameter). View the full article
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