Поиск по:www.astronomy.com -
Поискать по всем серверам
На этой странице приведены все страницы сервера www.astronomy.com ,которые мы индексируем. Показаны документы 1521 - 1540 из 10336.
Упорядочить по:
URL
|
дате изменения
1521. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BE603E435-C00A-474E-9C27-21A45FF8D8C1%7D
. A 3-D image of an impact crater in the Nilosyrtis area on the martian surface shows long pipe-like ridges, fossilized evidence of ancient subsurface water flow. // Credit: NASA Mars Reconnaissance Orbiter
[
Сохраненная копия
]
Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BE603E435-C00A-474E-9C27-21A45FF8D8C1%7D -- 3.1 Кб -- 10.04.2016
Похожие документы
Похожие документы
1522. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BE0CC2AEA-2009-4B14-B9D3-AC5D3679B781%7D
. Here a high-resolution monochrome image has been combined with a lower-resolution enhanced-color image. The hollows appear in cyan, a result of their high reflectance and bluish color relative to other parts of the planet. The large pit in the center of the crater may be a volcanic vent, from which the orange material erupted. Credit: Courtesy of Science/AAAS
[
Сохраненная копия
]
Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BE0CC2AEA-2009-4B14-B9D3-AC5D3679B781%7D -- 3.5 Кб -- 10.04.2016
Похожие документы
Похожие документы
1523. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BDAF2A720-7A0D-4AB5-8784-429FA6F2995A%7D
. Figure 1: Top: Optical images of Scheila at three different epochs with different telescopes. Images of the triple dust tails were taken on the 12th and 19th of December 2010 using the Murikabushi Telescope. Bottom: Suprime-Cam on the Subaru Telescope captured this image of the linear structure on the 2nd of March 2011.
[
Сохраненная копия
]
Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BDAF2A720-7A0D-4AB5-8784-429FA6F2995A%7D -- 3.4 Кб -- 10.04.2016
Похожие документы
Похожие документы
1524. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BDA803A66-11BF-4AC3-B724-5C906DD54B2A%7D
Figure 3: Image showing the result of a vast number of computer simulations to reproduce the shape of Scheila's triple dust tails observed December 12, 2010. The researchers reasoned that the downrange plume and the conical impact ejecta produced the dust particles, which sunlight pushed away from the asteroid. ... The downrange plume explains the appearance of the prominent northern feature (1) while the conical impact ejecta explain the remaining two structures (2)(3). ...
[
Сохраненная копия
]
Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BDA803A66-11BF-4AC3-B724-5C906DD54B2A%7D -- 3.9 Кб -- 10.04.2016
Похожие документы
Похожие документы
1525. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BD35B425E-43E5-4E38-8BEB-88342553EF6C%7D
. False-color image from the Herschel Space Observatory of starburst galaxy GN20 1.5 billion years after the Big Bang or more than 12 billion years back into the history of the universe. This is a "firework" with an extreme, but short-lived, star-forming episode believed to be triggered by a major merger. Credit: ESA/GOODS-Herschel Team and R. Gobat
[
Сохраненная копия
]
Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BD35B425E-43E5-4E38-8BEB-88342553EF6C%7D -- 3.5 Кб -- 10.04.2016
Похожие документы
Похожие документы
1526. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BD149A6DA-614C-4695-87BD-BF05DA389F42%7D
. Antennae Galaxies composite of ALMA and Hubble observations. Credit: ALMA (ESO/NAOJ/NRAO). Visible light image: NASA/ESA Hubble Space Telescope
[
Сохраненная копия
]
Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BD149A6DA-614C-4695-87BD-BF05DA389F42%7D -- 3.0 Кб -- 10.04.2016
Похожие документы
Похожие документы
1527. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BCEEDB5CE-F59E-4F5B-817F-D8E1332B36BC%7D
. A cross-section of Earth's interior shows the outer crust, the hot gooey mantle, the liquid outer core, and the solid, frozen inner core (gray). Graphic: Calvin J. Hamilton
[
Сохраненная копия
]
Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BCEEDB5CE-F59E-4F5B-817F-D8E1332B36BC%7D -- 3.0 Кб -- 10.04.2016
Похожие документы
Похожие документы
1528. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BB278A1A5-2269-485D-A441-CAC1B741AFDE%7D
. Artist's view of a dust torus surrounding the accretion disk and the central black hole in active galactic nuclei. Credit: NASA E/PO - Sonoma State University, Aurore Simonnet
[
Сохраненная копия
]
Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BB278A1A5-2269-485D-A441-CAC1B741AFDE%7D -- 3.0 Кб -- 10.04.2016
Похожие документы
Похожие документы
1529. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BAB908935-B1B5-4782-BE62-DA64FED6BD5D%7D
. The Pioneer Venus Orbiter captured this ultraviolet image of Venus' clouds February 26, 1979. NASA
[
Сохраненная копия
]
Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BAB908935-B1B5-4782-BE62-DA64FED6BD5D%7D -- 2.9 Кб -- 10.04.2016
Похожие документы
Похожие документы
1530. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B9DC8DB28-4026-4338-B538-8F5924971D39%7D
These images (insets) produced by the Lyman Alpha Mapping Project (LAMP) aboard NASA's Lunar Reconnaissance Orbiter reveal features at the Moon's northern and southern poles in the regions that lie in perpetual darkness. They show many permanently shadowed regions, or PSRs, are darker at far-ultraviolet wavelengths (top) and redder than nearby surface areas that receive sunlight (bottom). ...
[
Сохраненная копия
]
Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B9DC8DB28-4026-4338-B538-8F5924971D39%7D -- 4.0 Кб -- 10.04.2016
Похожие документы
Похожие документы
1531. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B9C80017B-E1ED-4109-BD64-9D6318A081A6%7D
. These two panels show the Snake Nebula as photographed by the Spitzer and Herschel space telescopes. At mid-infrared wavelengths (the upper panel taken by Spitzer), the thick nebular material blocks light from more distant stars. At far-infrared wavelengths, however (the lower panel taken by Herschel), the nebula glows due to emission from cold dust. The two boxed regions, P1 and P6, were examined in more detail by the Submillimeter Array (SMA). Spitzer/GLIMPSE/MIPS, Herschel/HiGal, Ke Wang (ESO)
[
Сохраненная копия
]
Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B9C80017B-E1ED-4109-BD64-9D6318A081A6%7D -- 3.8 Кб -- 10.04.2016
Похожие документы
Похожие документы
1532. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B94E5E841-F057-49D3-99AF-9E5B75F5E864%7D
. Figure 4: Orbits of the impacting asteroid and Scheila December 3, 2010, assuming an impact angle of 45ТА relative to the surface normal vector. Top: Face-on view, projected on the ecliptic plane. Bottom: Edge-on view, projected on the X-Z plane.
[
Сохраненная копия
]
Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B94E5E841-F057-49D3-99AF-9E5B75F5E864%7D -- 3.2 Кб -- 10.04.2016
Похожие документы
Похожие документы
1533. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B878D1F63-8871-4717-9960-3471597C476F%7D
This image, obtained during the late commissioning phase of the GeMS adaptive optics system, with the Gemini South AO Imager (GSAOI) on the night of December 28, 2012, reveals exquisite details in the outskirts of the Orion Nebula. ... In this image, the blue spots are clouds of gaseous iron "bullets" being propelled at supersonic speeds from a region of massive star formation outside, and below, this image's field of view. ... Credit: Gemini Observatory/AURA ...
[
Сохраненная копия
]
Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B878D1F63-8871-4717-9960-3471597C476F%7D -- 4.4 Кб -- 10.04.2016
Похожие документы
Похожие документы
1534. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B854836DE-B625-4778-B632-A81A621C7A72%7D
. Images of areas of 10ТА in radius around the nova MAXI J1409-619. A celestial body that was not observed on October 12 shone bright on the 17th. JAXA/RIKEN/MAXI team
[
Сохраненная копия
]
Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B854836DE-B625-4778-B632-A81A621C7A72%7D -- 3.1 Кб -- 10.04.2016
Похожие документы
Похожие документы
1535. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B7C8C0E6F-ED2F-45E2-820B-5207EA5D4431%7D
. Jupiter (right) and the Galilean satellites (right to left) Io, Europa, Ganymede, and Callisto. Cutaways show the interior states of Ganymede and Callisto after many impacts by icy planetesimals during the Late Heavy Bombardment. Colors represent density, with black showing the rocky core (with a density 3 g/cm^3), blue showing mixed ice and rock (densities 1.8 to 1.9 g/cm^3) and white showing rock-free ice. SwRI, San Antonio, Texas
[
Сохраненная копия
]
Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B7C8C0E6F-ED2F-45E2-820B-5207EA5D4431%7D -- 3.7 Кб -- 10.04.2016
Похожие документы
Похожие документы
1536. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B7C256B04-8185-4210-BB03-A28276D5FAEC%7D
A set of images of the Venus south polar vortex in infrared light (at 3.8 microns) acquired by the Visible and Infrared Thermal Imaging Spectrometer instrument on ESA's Venus Express spacecraft. The images show the temperature of the cloud tops at about 40 miles (65 kilometers). A darker region corresponds to higher temperature and thus lower altitude. The center of the vortex, at a temperature of about 250 kelvin, is the deepest zone, exhibiting the highest temperature. ...
[
Сохраненная копия
]
Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B7C256B04-8185-4210-BB03-A28276D5FAEC%7D -- 3.9 Кб -- 10.04.2016
Похожие документы
Похожие документы
1537. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B5CA464F9-8B67-4BE5-9DDB-BEB870CF5090%7D
This image from VISTA is a tiny part of the VISTA Variables in the Via Lactea (VVV) survey that is systematically studying the central parts of the Milky Way in infrared light. On the right lies the globular star cluster UKS 1 and on the left lies a much less conspicuous new discovery, VVV CL001 тАФ a previously unknown globular. The new globular appears as a faint grouping of stars about 25% of the width of the image from the left edge, and about 60% of the way from bottom to top. ...
[
Сохраненная копия
]
Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B5CA464F9-8B67-4BE5-9DDB-BEB870CF5090%7D -- 3.9 Кб -- 10.04.2016
Похожие документы
Похожие документы
1538. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B55A17B6C-1552-4551-AD4D-C35FD9D3FE13%7D
. This image combines Hubble observations of M106 with additional information captured by amateur astronomers Robert Gendler and Jay GaBany. Gendler combined Hubble data with his own observations to produce this stunning color image. // NASA, ESA, the Hubble Heritage Team (STScI/AURA), and R. Gendler (for the Hubble Heritage Team). Acknowledgment: J. GaBany
[
Сохраненная копия
]
Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B55A17B6C-1552-4551-AD4D-C35FD9D3FE13%7D -- 3.5 Кб -- 10.04.2016
Похожие документы
Похожие документы
1539. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B55994D1F-B190-425E-977C-BDA3492FE13C%7D
. Global mosaic of VIMS infrared images acquired during the nominal and equinox Cassini mission. Differences in composition translate into subtle differences of colors in this mosaic, revealing the diversity of terrains on Titan, such as the brownish equatorial dune fields or the bright elevated terrains. Credit: JPL/NASA/Univ. of Arizona/CNRS/LPGNantes
[
Сохраненная копия
]
Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B55994D1F-B190-425E-977C-BDA3492FE13C%7D -- 3.4 Кб -- 10.04.2016
Похожие документы
Похожие документы
1540. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B42768811-0E59-4800-B2AF-F487D04FDE71%7D
Here, a smooth particle hydrodynamics (SPH) simulation, in which matter is represented as particles, is used to model tidal stripping from a Titan-sized satellite consisting of 45 percent ice in an outer mantle and 55 percent silicate and metal in an inner core. The frames show material stripped from the satellite after [left] 8 simulated hours and [right] 25 simulated hours, assuming a fixed satellite orbit indicated by the outer dashed circle. ...
[
Сохраненная копия
]
Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B42768811-0E59-4800-B2AF-F487D04FDE71%7D -- 4.6 Кб -- 10.04.2016
Похожие документы
Похожие документы