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На этой странице приведены все страницы сервера www.astronomy.com ,которые мы индексируем. Показаны документы 221 - 240 из 10336.

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221. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BCFA61116-E460-4981-8086-8FF1A2BB75F9%7D

. The elevation profiles made by the laser altimeter on board MESSENGER from the northern hemisphere of Mercury (the warmer the color, the higher in elevation). Scientists used these high-precision range measurements to determine Mercury s rotation. NASA/Johns Hopkins University Applied Physics Laboratory/Carnegie Institution of Washington/DLR

[ Сохраненная копия ] Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BCFA61116-E460-4981-8086-8FF1A2BB75F9%7D -- 3.5 Кб -- 10.04.2016
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222. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B78BE150D-226A-42A8-B961-D10F343BDD52%7D

. Infrared images of Uranus (1.6 and 2.2 microns) obtained August 6, 2014, with adaptive optics on the 10-meter Keck telescope. The white spot is an extremely large storm that was brighter than any feature ever recorded on the planet in the 2.2 micron band. The cloud rotating into view at the lower-right limb grew into the large storm that was seen by amateur astronomers at visible wavelengths. Imke de Pater (UC Berkeley) Keck Observatory images

[ Сохраненная копия ] Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B78BE150D-226A-42A8-B961-D10F343BDD52%7D -- 3.7 Кб -- 10.04.2016
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223. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B5EB69217-CFAC-4071-8592-127DD5AB7251%7D

. This view of Mercury, the innermost planet in our solar system, was obtained during the first flyby of MESSENGER in 2008 and is a mosaic constructed from hundreds of individual images. NASA/Johns Hopkins University Applied Physics Laboratory/Carnegie Institution of Washington/DLR

[ Сохраненная копия ] Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B5EB69217-CFAC-4071-8592-127DD5AB7251%7D -- 3.4 Кб -- 10.04.2016
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224. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B5292EBF9-1E71-4627-92EA-EFE1AA04C2CA%7D

. Visualization of the Venus Express aerobraking maneuver. ESAтАУC. Carreau

[ Сохраненная копия ] Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B5292EBF9-1E71-4627-92EA-EFE1AA04C2CA%7D -- 2.9 Кб -- 10.04.2016
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225. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B24719D43-988E-4CAA-9D0D-3F9848816B51%7D

. NASA s Cassini spacecraft captured this view of the planet Uranus, the mission's first, on April 11, 2014. Distant Uranus is a small bluish orb here, barely resolved by Cassini's camera. NASA/JPL-Caltech/Space Science Institute

[ Сохраненная копия ] Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B24719D43-988E-4CAA-9D0D-3F9848816B51%7D -- 3.3 Кб -- 10.04.2016
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226. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B03898BFB-2DBB-49AC-B67A-F462A552FA97%7D

What if we could determine if a given star is likely to host a planetary system like our own by breaking down its light into a single high-resolution spectrum and analyzing it? ... The dark bands result from specific chemical elements in the star s outer layer, like hydrogen or iron, absorbing specific frequencies of light. By carefully measuring the width of each dark band, astronomers can determine just how much hydrogen, iron, calcium, and other elements are present in a distant star. ...

[ Сохраненная копия ] Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B03898BFB-2DBB-49AC-B67A-F462A552FA97%7D -- 4.5 Кб -- 10.04.2016
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227. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BFB21ABA0-6A7B-4DA7-A72F-45FA54B451C8%7D

. What astronomers once thought were two blazar families may in fact be one, as shown in this artist's concept. Energy stored in the black hole during its salad days of intense accretion may later be tapped by the blazar to continue its high-energy emissions long after this gas has been depleted. NASA's Goddard Space Flight Center

[ Сохраненная копия ] Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BFB21ABA0-6A7B-4DA7-A72F-45FA54B451C8%7D -- 3.4 Кб -- 10.04.2016
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228. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BF43C4A7B-5275-4D99-A6C8-4FC42D9D2F4C%7D

. Scientists using New Horizons images of Pluto s surface to make 3-D topographic maps have discovered that two of Pluto s mountains, informally named Wright Mons and Piccard Mons, could possibly be ice volcanoes. The color is shown to depict changes in elevation, with blue indicating lower terrain and brown showing higher elevation; green terrains are at intermediate heights. NASA/Johns Hopkins University Applied Physics Laboratory/Southwest Research Institute

[ Сохраненная копия ] Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BF43C4A7B-5275-4D99-A6C8-4FC42D9D2F4C%7D -- 3.8 Кб -- 10.04.2016
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229. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BEB627ED7-24FC-40AB-AE19-A657907880B6%7D

The informally named feature Wright Mons, located south of Sputnik Planum on Pluto, is an unusual feature that s about 100 miles (160 kilometers) wide and 13,000 feet (4km) high. It displays a summit depression (visible in the center of the image) that's approximately 35 miles (56km) across, with a distinctive hummocky texture on its sides. The rim of the summit depression also shows concentric fracturing. ...

[ Сохраненная копия ] Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BEB627ED7-24FC-40AB-AE19-A657907880B6%7D -- 4.3 Кб -- 10.04.2016
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230. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BD585DEF1-01B7-4D55-BE26-155F29DFB0C9%7D

. Brilliant Venus passed to the upper right of Jupiter after sunset March 12, 2012. The two planets repeat their close encounter in late June and early July. Alan Dyer

[ Сохраненная копия ] Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BD585DEF1-01B7-4D55-BE26-155F29DFB0C9%7D -- 3.1 Кб -- 10.04.2016
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231. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BA3AE58C4-A957-4753-88CC-21F6179E6A45%7D

. Uranus lies among the stars of southern Pisces at opposition October 11/12. Find it with naked eyes or binoculars; a telescope shows its small disk. Astronomy : Kellie Jaeger

[ Сохраненная копия ] Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BA3AE58C4-A957-4753-88CC-21F6179E6A45%7D -- 3.1 Кб -- 10.04.2016
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232. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B91F39394-89F9-436F-A818-D24B6E5429BE%7D

. Brilliant Venus passed a few degrees to Jupiter s upper right in evening twilight March 14, 2012. The two worlds will appear even closer during a return engagement in late June. Jamie Cooper

[ Сохраненная копия ] Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B91F39394-89F9-436F-A818-D24B6E5429BE%7D -- 3.2 Кб -- 10.04.2016
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233. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B87AE14E0-6103-4382-9BAF-E7720E42F4A0%7D

. The stars of the Beehive Cluster (M44) made a stunning backdrop for Venus on July 3, 2013. The planet revisits the cluster June 12 and 13. Luis Argerich

[ Сохраненная копия ] Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B87AE14E0-6103-4382-9BAF-E7720E42F4A0%7D -- 3.1 Кб -- 10.04.2016
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234. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B681C192F-6C36-4535-BBC2-6C736B3BF3BA%7D

. The morning star gleams at its brightest of the year September 21, joined by Jupiter and Mars in the predawn eastern sky. Astronomy : Roen Kelly

[ Сохраненная копия ] Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B681C192F-6C36-4535-BBC2-6C736B3BF3BA%7D -- 3.1 Кб -- 10.04.2016
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235. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B593366B1-7EB1-4E5A-B742-490704BF3B2C%7D

. You can find mission nebula NGC 3199, which lies in Carina the Keel, 4.4ТА southeast of magnitude 3.5 Phi (Я?) Velorum. Astronomy: Roen Kelly

[ Сохраненная копия ] Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B593366B1-7EB1-4E5A-B742-490704BF3B2C%7D -- 3.0 Кб -- 10.04.2016
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236. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B5134AD51-5E46-4C5D-953A-30CAF6F7F01B%7D

. Artist's impression of a volcano erupting on Venus. Whether Venus really is active today is a hot topic in planetary science. ESA - AOES Medialab

[ Сохраненная копия ] Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B5134AD51-5E46-4C5D-953A-30CAF6F7F01B%7D -- 3.1 Кб -- 10.04.2016
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237. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B1DAEF056-7F79-44C8-BAEB-7B14E0730758%7D

. Venus, Mars, and Jupiter create dramatic scenes throughout October. On the 28th, the three form a tight triangle. Astronomy : Kellie Jaeger

[ Сохраненная копия ] Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B1DAEF056-7F79-44C8-BAEB-7B14E0730758%7D -- 3.1 Кб -- 10.04.2016
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238. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B16499A52-AD35-409C-8A85-6D0AB2E47BB5%7D

. Venus and Jupiter lie within 1 of each other July 1. Coincidentally, both then appear 32" across through a telescope. Astronomy : Roen Kelly

[ Сохраненная копия ] Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B16499A52-AD35-409C-8A85-6D0AB2E47BB5%7D -- 3.1 Кб -- 10.04.2016
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239. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B0735FBD2-1F66-4DD5-99EB-515E3CB8D3BB%7D

. Evidence for active volcanoes on Venus

[ Сохраненная копия ] Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B0735FBD2-1F66-4DD5-99EB-515E3CB8D3BB%7D -- 2.7 Кб -- 10.04.2016
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240. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BB41FC571-4929-4888-A4E1-1670FACB8EDD%7D

. Artist s conception of Kepler 186f, an Earth-sized exoplanet in the habitable zone of its star. Stellar systems like this are prime targets for a new SETI program sponsored by the Breakthrough Prize Foundation. NASA

[ Сохраненная копия ] Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BB41FC571-4929-4888-A4E1-1670FACB8EDD%7D -- 3.2 Кб -- 10.04.2016
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