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На этой странице приведены все страницы сервера www.astronomy.com ,которые мы индексируем. Показаны документы 1561 - 1580 из 10336.

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1561. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BB53A60E7-D0F3-4559-BF23-19EBB52F8B5B%7D

. An artist's conception of 2007 OR10, nicknamed Snow White. Astronomers suspect that its rosy color is due to the presence of irradiated methane. Image credit: NASA

[ Сохраненная копия ] Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BB53A60E7-D0F3-4559-BF23-19EBB52F8B5B%7D -- 3.0 Кб -- 10.04.2016
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1562. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B9F4F0E9C-D7F4-42D7-8325-868ABE2B3967%7D

. The optical image of TN J0924-2201, a very distant radio galaxy at z = 5.19, obtained with the Hubble Space Telescope. Credit: NASA/STScI/NAOJ

[ Сохраненная копия ] Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B9F4F0E9C-D7F4-42D7-8325-868ABE2B3967%7D -- 3.0 Кб -- 10.04.2016
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1563. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B9D336836-6859-4D8D-9B0F-916C73CA8F9C%7D

. Spicules on the Sun, as observed by the Solar Dynamics Observatory. These bursts of gas jet off the surface of the sun at 150,000 miles (240,000 kilometers) per hour and contain gas that reaches temperatures over a million degrees. NASA Goddard/SDO/AIA

[ Сохраненная копия ] Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B9D336836-6859-4D8D-9B0F-916C73CA8F9C%7D -- 3.2 Кб -- 10.04.2016
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1564. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B8D24D42E-7F17-454A-9975-3301BC519538%7D

. The densest galaxy in the nearby universe may have been found. This galaxy weighs more than 200 million Suns, over half of which is concentrated within a radius of just 80 light-years. The density of stars in that region is 15,000 times greater than found in Earth's neighborhood in the Milky Way. Chandra, Hubble, and ground-based telescopes were used to discover and study this galaxy. X-ray: NASA/CXC/MSU/J.Strader et al, Optical: NASA/STScI

[ Сохраненная копия ] Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B8D24D42E-7F17-454A-9975-3301BC519538%7D -- 3.8 Кб -- 10.04.2016
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1565. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B8748E288-F4FE-49F6-B88F-77F02E7CFFDA%7D

. One of three discovery images of 2011 QF99 taken from CFHT on October 24, 2011 (2011 QF99 is inside the green circle). This is the first of three images of the same patch of sky, taken one hour apart, that were then compared to find moving light-sources. // Univ. of British Columbia

[ Сохраненная копия ] Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B8748E288-F4FE-49F6-B88F-77F02E7CFFDA%7D -- 3.3 Кб -- 10.04.2016
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1566. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B856B641A-213B-486B-9744-EAADD97C308B%7D

. The region of the Hubble Deep Field where HDF850.1 is located. The cross indicates the submillimeter galaxy's position. For observations with ordinary visible light telescopes, such as the Hubble Space Telescope, the galaxy is completely invisible. Image credit: STScI/NASA/F. Walter (MPIA)

[ Сохраненная копия ] Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B856B641A-213B-486B-9744-EAADD97C308B%7D -- 3.3 Кб -- 10.04.2016
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1567. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B76FA83E8-43DA-4CD0-A1B1-4B1B2BCDE38A%7D

. Full Dark Energy Camera image of the Fornax cluster of galaxies, which lies about 60 million light years from Earth. The center of the cluster is the clump of galaxies in the upper portion of the image. The prominent galaxy in the lower right of the image is the barred spiral galaxy NGC 1365. // Credit: Dark Energy Survey Collaboration

[ Сохраненная копия ] Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B76FA83E8-43DA-4CD0-A1B1-4B1B2BCDE38A%7D -- 3.4 Кб -- 10.04.2016
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1568. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B71712FF4-D982-45E4-8757-145FE57B2377%7D

. Artist's impression of the Cluster mission. Credit: ESA

[ Сохраненная копия ] Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B71712FF4-D982-45E4-8757-145FE57B2377%7D -- 2.8 Кб -- 10.04.2016
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1569. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B6F222280-7341-4768-9D60-EAA4CEE6E523%7D

. The Transit of Venus of June 6, 2012, as seen from Wiltshire in the United Kingdom. // Credit: Grant Privett

[ Сохраненная копия ] Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B6F222280-7341-4768-9D60-EAA4CEE6E523%7D -- 2.9 Кб -- 10.04.2016
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1570. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B6A02B877-69D2-4FFF-8253-62D62F3ADF08%7D

. An infrared image of Dragonfish association, showing the shell of hot gas. NASA/JPL- Caltech/GLIMPSE Team/Mubdi Rahman

[ Сохраненная копия ] Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B6A02B877-69D2-4FFF-8253-62D62F3ADF08%7D -- 2.9 Кб -- 10.04.2016
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1571. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B665894CF-C156-4DBC-BD6C-CC245A553AA2%7D

. This mosaic of images from the Mast Camera (Mastcam) instrument on NASA's Curiosity Mars rover shows a series of sedimentary deposits in the Glenelg area of Gale Crater, from a perspective in Yellowknife Bay looking toward west-northwest. NASA/JPL-Caltech/MSSS

[ Сохраненная копия ] Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B665894CF-C156-4DBC-BD6C-CC245A553AA2%7D -- 3.3 Кб -- 10.04.2016
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1572. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B6524B68C-2CC1-442E-9740-A503CD4D7A25%7D

. Voyager 1 captured this mosaic of our solar system at almost 13 billion miles (20 billion kilometers) from Earth and 32ТА degrees above the plane of the solar system. Although our systemт??s organization is more often the exception than the rule, a recent study shows that the high degree of alignment of our system might well be the norm. NASA/JPL

[ Сохраненная копия ] Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B6524B68C-2CC1-442E-9740-A503CD4D7A25%7D -- 3.5 Кб -- 10.04.2016
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1573. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B5F807AB6-4394-44A5-93BE-2D3AD863C96C%7D

. In the newly discovered type of AGN, the disk and torus surrounding the black hole are so deeply obscured by gas and dust that no visible light escapes, making them very difficult to detect. This illustration shows the scene from a more distant perspective. Aurore Simonnet (Sonoma State University)

[ Сохраненная копия ] Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B5F807AB6-4394-44A5-93BE-2D3AD863C96C%7D -- 3.3 Кб -- 10.04.2016
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1574. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B52756E37-C425-4C04-A2BB-DF8FFBF292E9%7D

This photo illustration depicts a view of the night sky just before the predicted merger between our Milky Way Galaxy and the neighboring Andromeda Galaxy. About 3.75 billion years from now, Andromeda's disk fills the field of view and its gravity begins to create tidal distortions in the Milky Way. The view is inspired by dynamical computer modeling of the future collision between the two galaxies. ...

[ Сохраненная копия ] Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B52756E37-C425-4C04-A2BB-DF8FFBF292E9%7D -- 4.0 Кб -- 10.04.2016
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1575. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B3EAF70D3-759E-4E15-BF6B-1DAD3DE9425A%7D

This image shows a standard prediction for the dark matter distribution within about 1 million light years of the Milky Way galaxy, which is expected to be swarming with thousands of small dark matter clumps called `halos'. ... Until now, there was no observational evidence that dark matter actually clumps this way, raising concerns that our understanding of the cosmos was flawed in a fundamental way. ...

[ Сохраненная копия ] Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B3EAF70D3-759E-4E15-BF6B-1DAD3DE9425A%7D -- 4.4 Кб -- 10.04.2016
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1576. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B3B486347-2D55-45D7-9DA4-6646DC5A2DA2%7D

. Artist's rendition of the protoplanetary disk around J 1604. // The Graduate University for Advanced Studies, Japan

[ Сохраненная копия ] Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B3B486347-2D55-45D7-9DA4-6646DC5A2DA2%7D -- 2.9 Кб -- 10.04.2016
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1577. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B31271431-A6C6-4FFB-9ABD-0511EF08CF18%7D

. In this artist's conception, Jupiter's migration through the solar system has swept asteroids out of stable orbits, sending them careening into one another. As the gas giant planets migrated, they stirred the contents of the solar system. Objects from as close to the Sun as Mercury and as far out as Neptune all collected in the main asteroid belt, leading to the diverse composition we see today. David A. Aguilar (CfA)

[ Сохраненная копия ] Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B31271431-A6C6-4FFB-9ABD-0511EF08CF18%7D -- 3.7 Кб -- 10.04.2016
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1578. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B300B2436-F429-4993-9972-B1791816AA27%7D

Studies of oscillation frequencies of many stars with very high precision gives insights into stellar evolution by knowing how the cores of stars change (starting in the bottom left corner in the sequence above) from hydrogen fusion-burning cores to helium fusion-burning cores, with intermediate stages where hydrogen fusion-burning shells expand into red giant sizes. A Hydrogen shell fusion star and a Helium core fusion star are indistinguishable when looking only at their surface properties. ...

[ Сохраненная копия ] Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B300B2436-F429-4993-9972-B1791816AA27%7D -- 4.1 Кб -- 10.04.2016
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1579. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B2FD153AF-5093-4D74-B956-FBD1E7B7A08B%7D

. This spectacular view of the crater Degas was obtained as a high-resolution targeted observation (296 feet [90 meters] per pixel). Impact melt coats its floor, and as the melt cooled and shrank, it formed the cracks observed across the crater. For context, Mariner 10т??s view of Degas is shown at left. Degas is 32 miles (52 kilometers) in diameter and is centered at 37.1ТА N, 232.8ТА E. NASA/Johns Hopkins University Applied Physics Laboratory/Carnegie Institution of Washington

[ Сохраненная копия ] Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B2FD153AF-5093-4D74-B956-FBD1E7B7A08B%7D -- 3.8 Кб -- 10.04.2016
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1580. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B2864B7AA-04B2-4148-9650-6AA26FF23C71%7D

. Electron microscope image showing the 700-million-year-old martian clay veins containing boron (100 ТЕm = one tenth of a millimeter). // Institute of Astronomy, Univ. of Hawaii

[ Сохраненная копия ] Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B2864B7AA-04B2-4148-9650-6AA26FF23C71%7D -- 3.1 Кб -- 10.04.2016
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