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На этой странице приведены все страницы сервера www.astronomy.com ,которые мы индексируем. Показаны документы 621 - 640 из 10336.

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621. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B20903DEA-2F96-4DDB-830E-46F92B8E5072%7D
. NASA's Pluto-bound New Horizons spacecraft snapped this image of Jupiter and its moon Io when the two crossed paths in 2008. Astronomers say Jupiter could have ejected another planet from our solar system without losing its moons. NASA/JHU-APL/Southwest Research Institute
[ Сохраненная копия ]  Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B20903DEA-2F96-4DDB-830E-46F92B8E5072%7D -- 3.3 Кб -- 10.04.2016
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622. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B00DA0300-E212-4E9E-ACF4-C9179CF113B5%7D
. The Cat's Paw Nebula (NGC 6334) comes alive in this infrared image from the Spitzer Space Telescope. A new study of this nebula finds that magnetic fields influence star formation on a variety of scales, from hundreds of light-years down to a fraction of a light-year. In this representative color photo red shows light at a wavelength of 8 microns, green is 4.5 microns, and blue is 3.6 microns. S. Willis (CfA); NASA/JPL-Caltech/SSC
[ Сохраненная копия ]  Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B00DA0300-E212-4E9E-ACF4-C9179CF113B5%7D -- 3.7 Кб -- 10.04.2016
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623. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BCA2BE3C2-AB19-4152-AB8E-392647B8D3BA%7D
. Chandra data show the supermassive black hole at the center of NGC 5813 has erupted multiple times over 50 million years. NGC 5813 is the central component of a group of galaxies called the NGC 5813 Group that is immersed in an enormous reservoir of hot gas. X-ray: NASA/CXC/SAO/S.Randall, et al.; Optical: SDSS
[ Сохраненная копия ]  Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BCA2BE3C2-AB19-4152-AB8E-392647B8D3BA%7D -- 3.4 Кб -- 10.04.2016
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624. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BC8091511-E8F6-4D33-96DC-5DB3F7F45740%7D
. ESO s Very Large Telescope in Chile has captured the most detailed image ever taken of the Medusa Nebula (also known as Abell 21 and Sharpless 2-274). As the star at the heart of this nebula made its final transition into retirement, it shed its outer layers into space, forming this colorful cloud. The image foreshadows the final fate of the Sun, which will eventually also become an object of this kind. ESO
[ Сохраненная копия ]  Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BC8091511-E8F6-4D33-96DC-5DB3F7F45740%7D -- 3.7 Кб -- 10.04.2016
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625. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BC4D598BF-4619-4EE0-A7AD-3AEBA0FE3535%7D
The galaxy cluster called MOO J1142+1527 can be seen here as it existed when light left it 8.5 billion years ago. The red galaxies at the center of the image make up the heart of the galaxy cluster. ... In addition to galaxies, clusters also contain a reservoir of hot gas with temperatures in the tens of millions of degrees. CARMA was used to detect this gas and to determine the mass of this cluster. NASA/JPL-Caltech/Gemini/CARMA ...
[ Сохраненная копия ]  Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BC4D598BF-4619-4EE0-A7AD-3AEBA0FE3535%7D -- 4.6 Кб -- 10.04.2016
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626. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B856681FC-A9F5-4C4C-A8C1-05675EA43E7D%7D
. The smallest supermassive black hole ever detected in the center of a galaxy has been identified using observations with Chandra and the 6.5-meter Clay Telescope. The host galaxy for the tiny heavyweight black hole is a dwarf disk galaxy called RGG 118, shown in an image from the Sloan Digital Sky Survey. The Chandra image of the galaxy's center shows hot gas near the black hole. X-ray: NASA/CXC/Univ. of Michigan/V. F. Baldassare, et al.; Optical: SDSS
[ Сохраненная копия ]  Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B856681FC-A9F5-4C4C-A8C1-05675EA43E7D%7D -- 3.7 Кб -- 10.04.2016
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627. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B6A7BCA82-6685-4434-8F39-BB78E7FA742E%7D
. This natural color view from NASA's Mars Exploration Rover Opportunity shows "Lunokhod 2 Crater," which lies south of Solander Point on the west rim of Endeavour Crater. NASA/JPL-Caltech/Cornell/Arizona State Univ.
[ Сохраненная копия ]  Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B6A7BCA82-6685-4434-8F39-BB78E7FA742E%7D -- 3.2 Кб -- 10.04.2016
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628. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B5D6A9A31-A6B2-4682-A680-D438EDB8E37E%7D
. An intriguing object has been found in one of the spiral arms of the galaxy NGC 2276. This source, called NGC 2276-3c, appears to be an intermediate-mass black hole. According to X-ray and radio data, NGC 2276-3c contains about 50,000 times the mass of the Sun. X-ray: NASA/CXC/SAO/M.Mezcua et al NASA/CXC/INAF/A.Wolter et al; Optical: NASA/STScI and DSS; Inset: Radio: EVN/VLBI
[ Сохраненная копия ]  Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B5D6A9A31-A6B2-4682-A680-D438EDB8E37E%7D -- 3.6 Кб -- 10.04.2016
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629. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B51E3A1F4-CE29-4B45-928A-4F0551428FC0%7D
. An artist s concept shows a celestial body about the size of our moon slamming at great speed into a body the size of Mercury. NASA/JPL-Caltech
[ Сохраненная копия ]  Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B51E3A1F4-CE29-4B45-928A-4F0551428FC0%7D -- 3.0 Кб -- 10.04.2016
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630. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B4C53871D-929F-4443-B333-DB0146B7BB68%7D
. A massive cluster of galaxies, called SpARCS1049+56, can be seen in this multi-wavelength view from NASA's Hubble and Spitzer space telescopes. NASA/STScI/ESA/JPL-Caltech/McGill
[ Сохраненная копия ]  Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B4C53871D-929F-4443-B333-DB0146B7BB68%7D -- 3.1 Кб -- 10.04.2016
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631. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B47D70C68-D212-47E8-9EC6-0604FEA84832%7D
. A new Chandra image of M51 contains nearly a million seconds of observing time. The data reveal hundreds of point-like X-ray sources within what is nicknamed the "Whirlpool Galaxy." Most of these point sources are X-ray binary systems with either a neutron star or black hole orbiting a Sun-like star. The composite image consists of X-rays from Chandra (purple) and optical data from Hubble (red, green, and blue). X-ray: NASA/CXC/Wesleyan Univ./R.Kilgard, et al; Optical: NASA/STScI
[ Сохраненная копия ]  Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B47D70C68-D212-47E8-9EC6-0604FEA84832%7D -- 3.8 Кб -- 10.04.2016
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632. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B3A19D320-B261-4B0E-B78A-AE3132E9BD3F%7D
Rings of X-ray light centered on V404 Cygni, a binary system containing an erupting black hole (dot at center), were imaged by the X-ray Telescope aboard NASA's Swift satellite from June 30 to July 4. ... Color indicates the energy of the X-rays, with red representing the lowest (800 to 1,500 electron volts, eV), green for medium (1,500 to 2,500 eV), and the most energetic (2,500 to 5,000 eV) shown in blue. ... The dark lines running diagonally through the image are artifacts of the imaging system. ...
[ Сохраненная копия ]  Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B3A19D320-B261-4B0E-B78A-AE3132E9BD3F%7D -- 4.2 Кб -- 10.04.2016
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633. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B26822ECD-3BCA-4C23-86CA-C407C4C1C167%7D
. This composite of C/2013 A1 (Siding Spring) merges Swift UVOT images taken between May 27 and 29, 2014. Sunlight reflected from the comet's dust, which produces most of the light in this image, appears yellow; violet shows ultraviolet light produced by hydroxyl (OH), a molecular fragment of water. NASA/Swift/D. Bodewits (UMD), DSS
[ Сохраненная копия ]  Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B26822ECD-3BCA-4C23-86CA-C407C4C1C167%7D -- 3.5 Кб -- 10.04.2016
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634. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B26394131-4168-4273-AC85-B815F210AA32%7D
. A "radio phoenix" has been discovered using X-ray, radio, and optical data. This system contains the collision of two galaxy clusters located about 1.6 billion light years from Earth. The collision re-energized a regeneration of vast clouds of high-energy particles that primarily radiate at radio frequencies. Understanding how galaxy clusters grow over time, including through collisions, is important for cosmology. X-ray: NASA/CXC/Univ of Hamburg/F. de Gasperin et al; Optical: SDSS; Radio: NRAO/VLA
[ Сохраненная копия ]  Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B26394131-4168-4273-AC85-B815F210AA32%7D -- 3.8 Кб -- 10.04.2016
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635. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B25C9D0D4-449A-40D6-AC1B-1790D9464C60%7D
. These images show the central plane of a rotating disk orbiting a newly formed protostar (dark dot) formed in a 3-D model of the shock-triggered collapse of a molecular cloud of gas and dust. Density is shown on the left, while the x velocity plot on the right shows how the shock (outer edge) has injected fingers with motions that are responsible for producing the spin of the disk around the central protostar. Courtesy of Alan Boss
[ Сохраненная копия ]  Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B25C9D0D4-449A-40D6-AC1B-1790D9464C60%7D -- 3.7 Кб -- 10.04.2016
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636. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B1B69FEF2-FDE6-4A0C-B650-54269402F84A%7D
. Earth as seen July 6, 2015, from a distance of 1 million miles by a NASA scientific camera aboard the Deep Space Climate Observatory spacecraft. NASA
[ Сохраненная копия ]  Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B1B69FEF2-FDE6-4A0C-B650-54269402F84A%7D -- 3.0 Кб -- 10.04.2016
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637. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B0951465A-7467-4F80-8138-CF7A368F5DEF%7D
. The computer code used to produce the amazing visuals in Interstellar have revealed interesting properties about black holes. Paramount Pictures
[ Сохраненная копия ]  Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B0951465A-7467-4F80-8138-CF7A368F5DEF%7D -- 3.1 Кб -- 10.04.2016
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638. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B97BB3B05-EA3D-4F24-AC47-D839A9E030FB%7D
. X-rays from Chandra reveal giant holes, or cavities, in the hot gas that pervades the cluster. Massive filaments of gas and dust surround the X-ray cavities and may play a role in the extreme star formation seen in the cluster. X-ray: NASA/CXC/MIT/M.McDonald et al; Optical: NASA/STScI
[ Сохраненная копия ]  Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B97BB3B05-EA3D-4F24-AC47-D839A9E030FB%7D -- 3.4 Кб -- 10.04.2016
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639. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B75E733F7-12F5-48C8-835B-A5F29A91E156%7D
New images are being released to celebrate the International Year of Light 2015. ... M51: X-ray: NASA/CXC/SAO; UV: NASA/JPL-Caltech; Optical: NASA/STScI; IR: NASA/JPL-Caltech; SNR0519-69.0: X-ray: NASA/CXC/Rutgers/J.Hughes; Optical: NASA/STScI; MSH 11-62: X-ray: NASA/CXC/SAO/P.Slane et al; Optical: DSS; Radio: CSIRO/ATNF/ATCA; Cygnus A: X-ray: NASA/CXC/SAO; Optical: NASA/STScI; Radio: NSF/NRAO/AUI/VLA; RCW 86: X-ray: NASA/CXC/MIT/D.Castro et al, Optical: NOAO/AURA/NSF/CTIO ...
[ Сохраненная копия ]  Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B75E733F7-12F5-48C8-835B-A5F29A91E156%7D -- 4.4 Кб -- 10.04.2016
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640. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B51785F7C-61E2-4CF1-8CB0-0AD3DEAE3153%7D
. These image shows the difference between two sets of 48 combined 10-second exposures with New Horizons' Long Range Reconnaissance Imager (LORRI) camera, taken at 8:40 UTC and 10:25 UTC on June 26, 2015, from a range of 13.4 million miles (21.5 million kilometers) to Pluto. The known small moons, Nix, Hydra, Kerberos and Styx, are visible as adjacent bright and dark pairs of dots due to their motion in the 105 minutes between the two image sets. NASA/JHUAPL/SwRI
[ Сохраненная копия ]  Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B51785F7C-61E2-4CF1-8CB0-0AD3DEAE3153%7D -- 3.8 Кб -- 10.04.2016
[ Сохраненная копия ]  Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BA39B8D27-0923-45CF-BF76-B4E55A548E93%7D -- 3.8 Кб -- 10.04.2016
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