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1541. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B404763A0-C562-42CA-858D-588C47964C0E%7D
. NASA's decommissioned Upper Atmosphere Research Satellite fell back to Earth between 11:23 p.m. EDT September 23 and 1:09 a.m. September 24. NASA
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B404763A0-C562-42CA-858D-588C47964C0E%7D -- 3.0 Кб -- 10.04.2016
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1542. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B3B61385C-8555-4585-A460-19168957AD3B%7D
. Sunspot 1302 has already produced two X-flares (X1.4 on September 22 and X1.9 on September 24). Each of the dark cores in this image from SDO is larger than Earth, and the entire active region stretches more than 62,00 miles (100,000 km) from end to end. NASA/SDO/HMI
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B3B61385C-8555-4585-A460-19168957AD3B%7D -- 3.3 Кб -- 10.04.2016
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1543. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B376D66BB-A6A3-4E4A-AB2D-ADD17FB9789D%7D
. When the rimwall of IapetusтАЩ Malun crater broke off and plunged more than 5 miles (8 kilometers) to the crater floor, it surged an astonishing 22 miles (35kms) out from the base of the wall before finally coming to rest. WUSTL planetary scientists speculate that steep topography on the ice moon allows the ice to pick up enough speed to become slippery, even though temperatures on Iapetus are in liquid-nitrogen territory. Credit: NASA/JPL/Space Science Institute
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B376D66BB-A6A3-4E4A-AB2D-ADD17FB9789D%7D -- 3.7 Кб -- 10.04.2016
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1544. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B319109EC-5BC6-4D3B-BC50-669907E708D1%7D
. Figure 2: Sequence of events after an oblique impact: (a) Object impacts another and generates a shock wave; (b) and (c) increased development of two prominent features, i.e., a downrange plume and conical impact ejecta. The downrange plume results from the fragmentation or sometimes the evaporation of the impacting object while the conical impact ejecta come from the physical destruction of the impacted object when the shock wave spreads from the site of impact and scoops up materials from it.
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B319109EC-5BC6-4D3B-BC50-669907E708D1%7D -- 3.8 Кб -- 10.04.2016
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1545. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B289BAF54-F70D-45F3-837B-A98977A77370%7D
. This is a mosaic of the images covering the entire sky as observed by the Wide-field Infrared Survey Explorer (WISE), part of its All-Sky Data Release. Credit: NASA/JPL-Caltech/UCLA
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B289BAF54-F70D-45F3-837B-A98977A77370%7D -- 3.1 Кб -- 10.04.2016
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1546. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B1164509B-B3E2-4390-8C22-122D971127BD%7D
. This set of artist's concepts shows NASA's Mars Science Laboratory cruise capsule and NASA's Orion spacecraft, which is being built now at NASA's Johnson Space Center and will one day send astronauts to Mars. // NASA/JPL-Caltech/JSC
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B1164509B-B3E2-4390-8C22-122D971127BD%7D -- 3.2 Кб -- 10.04.2016
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1547. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B0FC35552-4838-493E-BCFF-BB7DBFA6EDE2%7D
. The solar system moves through a local galactic cloud at a speed of 50,000 mph, driving an interstellar wind of particles, which can be measured by Earth-orbiting or interplanetary spacecraft. NASA/Adler/UChicago/Wesleyan
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B0FC35552-4838-493E-BCFF-BB7DBFA6EDE2%7D -- 3.2 Кб -- 10.04.2016
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1548. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B0D60B2BE-53A4-429A-93EA-556827C0E482%7D
. The Radiation Assessment Detector on NASA's Curiosity Mars rover monitors high-energy atomic and subatomic particles coming from the Sun, distant supernovae, and other sources. // NASA/JPL-Caltech/SwRI
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B0D60B2BE-53A4-429A-93EA-556827C0E482%7D -- 3.1 Кб -- 10.04.2016
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1549. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B0C1272BB-1BB3-4E5D-BBC2-32082F484C2D%7D
. SwRI has concluded agreements with Virgin Galactic for a research seat on each of two suborbital flights; discussions are also under way for an additional charter mission involving up to six seats. Virgin Galactic will use its SpaceShip 2 to carry the researchers to altitudes as high as 350,000 feet. Photo courtesy Virgin Galactic
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B0C1272BB-1BB3-4E5D-BBC2-32082F484C2D%7D -- 3.4 Кб -- 10.04.2016
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1550. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B0A59DF46-7C8D-4002-9B8E-283BFD8434DA%7D
. This self-portrait of NASA's Mars rover Curiosity combines 66 exposures taken by the rover's Mars Hand Lens Imager (MAHLI) during the 177th martian day, or sol, of Curiosity's work on Mars (February. 3, 2013). NASA/JPL-Caltech/MSSS
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B0A59DF46-7C8D-4002-9B8E-283BFD8434DA%7D -- 3.3 Кб -- 10.04.2016
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1551. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B0878488B-A150-4F6E-804F-A7ED19C864EB%7D
. Gemini SouthтАЩs first-light image from GeMS/GSAOI shows extreme detail in the central part of the globular star cluster NGC 288. North is up, East is right.
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B0878488B-A150-4F6E-804F-A7ED19C864EB%7D -- 3.0 Кб -- 10.04.2016
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1552. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B0727A16C-12E3-4B30-94B7-D34CB47282A4%7D
. Approach image of Vesta contrasting southern hemisphere (lower right) with northern hemisphere (upper left). NASA/JPL-Caltech/UCLA/MPS/DLR/IDA
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B0727A16C-12E3-4B30-94B7-D34CB47282A4%7D -- 3.0 Кб -- 10.04.2016
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1553. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B06901546-12D2-491A-B779-162CED37BC06%7D
. This image shows the first-ever view of the magnetospheric plasma sheet in profile, as seen by the Interstellar Boundary Explorer (IBEX) from outside the magnetosphere. It shows the densest portions of the plasma sheet, largely following the modeled magnetic structure. Image courtesy of NASA/IBEX Science Team
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B06901546-12D2-491A-B779-162CED37BC06%7D -- 3.4 Кб -- 10.04.2016
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1554. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B01CE31F6-7EC5-48C2-9FEB-C002293329EE%7D
. This picture of the nebula around a rare yellow hypergiant star called IRAS 17163-3907 is the best ever taken of a star in this class and shows for the first time a huge dusty double shell surrounding the central hypergiant. The star and its shells resemble an egg white around a yolky center, leading astronomers to nickname the object the Fried Egg Nebula. ESO/E. Lagadec
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B01CE31F6-7EC5-48C2-9FEB-C002293329EE%7D -- 3.6 Кб -- 10.04.2016
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1555. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BF91A3E65-1845-4BEB-9B38-DF5875AF19E1%7D
. This artistтАЩs impression shows two galaxies in the early universe. The brilliant explosion on the left is a gamma-ray burst. The light from the burst travels through both galaxies on its way to Earth (outside the frame to the right). Analysis of observations of the light from this gamma-ray burst made using ESOтАЩs Very Large Telescope have shown that these two galaxies are remarkably rich in heavier chemical elements. Credit: ESO/L. Cal?зada
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BF91A3E65-1845-4BEB-9B38-DF5875AF19E1%7D -- 3.7 Кб -- 10.04.2016
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1556. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BE8EBDE39-7B72-4125-B782-E3801AAC81EB%7D
Kepler, the paparazzi of the celestial stars, takes snapshots of oscillations that can can be used to tell the size and age of the star. As a star "burns" hydrogen in fusion reactions, helium builds up in the star's core. Helium is more dense than hydrogen, and since waves travel more quickly through denser material, waves travel faster through the core as helium builds up there. ... Travis Metcalfe, National Center for Atmospheric Research ...
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BE8EBDE39-7B72-4125-B782-E3801AAC81EB%7D -- 4.0 Кб -- 10.04.2016
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1557. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BE6E10C79-9730-482B-B05B-C366467A6B9A%7D
. European ALMA antenna brings total on Chajnantor to 16. ESO/S. Rossi
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BE6E10C79-9730-482B-B05B-C366467A6B9A%7D -- 2.8 Кб -- 10.04.2016
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1558. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BD578F439-ED45-4B8B-A34A-53A0A1E9E500%7D
. Subaru Telescope's near-infrared image of the protoplanetary disk around the young star J 1604. A black circular mask covers the bright, saturated light from the central star. The gauges for distance are in astronomical units and arcseconds. Prominent features include the hole (white dotted line) in the disk; the arm extending over the hole (on the right); and the asymmetric dip (on the left). // Graduate Univ. for Advanced Studies and the National Astronomical Observatory of Japan
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BD578F439-ED45-4B8B-A34A-53A0A1E9E500%7D -- 3.8 Кб -- 10.04.2016
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1559. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BCAF448EC-8CF7-40D0-8E2F-5147A0D01CF4%7D
. Two images of SaturnтАЩs northern auroral oval made with the Ultraviolet Imaging Spectrometer (UVIS) instrument. The second image, made two hours after the first, shows the motion of the oval as the planet rotates. Credit: NASA/ESA and the Cassini UVIS team
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BCAF448EC-8CF7-40D0-8E2F-5147A0D01CF4%7D -- 3.3 Кб -- 10.04.2016
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1560. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BB702F25A-6278-4D94-9A92-ED29E46FD359%7D
. A graphical representation of the pear-shaped nucleus of an exotic atom. The shape of the nucleus could give clues to why the universe contains more matter than antimatter. // Liam Gaffney and Peter Butler, University of Liverpool
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BB702F25A-6278-4D94-9A92-ED29E46FD359%7D -- 3.2 Кб -- 10.04.2016
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