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2601. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B5A117EBE-2E72-4B41-BDFC-4E6ADFC5EE05%7D
. The Antares rocket clears the launch pad on its way to orbit. // NASA/Bill Ingalls
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B5A117EBE-2E72-4B41-BDFC-4E6ADFC5EE05%7D -- 2.8 Кб -- 10.04.2016
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2602. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B51385D14-E955-4779-82C4-6B69CD20BEC9%7D
. This artist's concept depicts red dwarf KOI-961 and its three planets, which are all smaller than Earth. The smallest of the three planets (pictured here in the foreground), called KOI-961.03, is about the size of Mars and is located the farthest from the star. The planet in the upper right is KOI-961.01, 0.78 times the radius of Earth. The planet closest to the star is KOI-961.02, with a radius 0.73 times Earth's. NASA/JPL-Caltech
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B51385D14-E955-4779-82C4-6B69CD20BEC9%7D -- 3.7 Кб -- 10.04.2016
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2603. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B4E6A9F16-A82B-40BA-811E-217DEBE4F25E%7D
. If astronomers could somehow pull planets out of the sky and analyze them in the laboratory, it might look something like this artistically altered image illustrating new research from NASA's Spitzer Space Telescope. The infrared observatory allows astronomers to study closely the atmospheres of hot Jupiter planets тАФ those outside our solar system that orbit near the blistering heat of their stars. // NASA/JPL-Caltech
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B4E6A9F16-A82B-40BA-811E-217DEBE4F25E%7D -- 3.6 Кб -- 10.04.2016
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2604. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B40373BF9-F188-40BE-8250-8F3E754FFBA8%7D
. During cryogenic testing, the mirrors will be subjected to temperatures dipping to -415ТАFahrenheit (-248ТА Celsius), permitting engineers to measure in detail how the shape of each mirror changes as it cools. NASA/MSFC/David Higginbotham/Emmett Given
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B40373BF9-F188-40BE-8250-8F3E754FFBA8%7D -- 3.3 Кб -- 10.04.2016
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2605. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B3A2E7053-3FA7-4F2D-8D1F-AA489EAAED14%7D
. The Boomerang Nebula, called the coldest place in the universe, reveals its true shape with ALMA. The background blue structure, as seen in visible light with the Hubble Space Telescope, shows a classic double-lobe shape with a very narrow central region. ALMA s resolution and ability to see the cold molecular gas reveals the nebula s more elongated shape, as seen in red. Bill Saxton; NRAO/AUI/NSF; NASA/Hubble; Raghvendra Sahai
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B3A2E7053-3FA7-4F2D-8D1F-AA489EAAED14%7D -- 3.7 Кб -- 10.04.2016
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2606. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B29BFD1F7-C747-4A7D-AC5B-13E260F9F221%7D
. SOHO's 2000th comet, spotted by a Polish amateur astronomer December 26, 2010. SOHO/Karl Battams
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B29BFD1F7-C747-4A7D-AC5B-13E260F9F221%7D -- 2.9 Кб -- 10.04.2016
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2607. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B1AD5EA07-09FE-4166-A669-F7D6982799D3%7D
. Artrist's impression of JUICE
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B1AD5EA07-09FE-4166-A669-F7D6982799D3%7D -- 2.7 Кб -- 10.04.2016
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2608. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B0F0AFF07-830D-4A24-8FD9-93E48305736F%7D
. The faint filaments of the giant supernova remnant known as the Cygnus Loop are visible in this image obtained with the wide-field view of the Mosaic camera on the WIYN 0.9-meter telescope. Because of its immense size, it contains several individually named objects, including NGC 6992 and IC 1340 on the left side as well as NGC 6960 and Pickering's Triangle on the right. // T. A. Rector (University of Alaska Anchorage)/WIYN/NOAO/AURA/NSF
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B0F0AFF07-830D-4A24-8FD9-93E48305736F%7D -- 3.7 Кб -- 10.04.2016
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2609. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B0F026B9B-8049-4846-8F58-9BA282E8ABDC%7D
. In the image at left, the galaxy in the center produced the gamma-ray burst. Hubble observed the galaxy June 13, 2013, and saw a near-infrared glow at the site of the burst, shown in the top righthand image. When Hubble observed the location again July 3, the source had faded, as shown in the lower righthand image. The dimming source is a decaying fireball of a new type of stellar blast called a kilonova. // NASA/ESA/N. Tanvir (University of Leicester)
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B0F026B9B-8049-4846-8F58-9BA282E8ABDC%7D -- 3.7 Кб -- 10.04.2016
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2610. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BFC0C40F7-91DF-4E73-ACED-E9DB4904A309%7D
. This computer-generated view depicts part of Mars at the boundary between darkness and daylight, with an area including Gale Crater beginning to catch morning light. Credit: NASA/JPL-Caltech
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BFC0C40F7-91DF-4E73-ACED-E9DB4904A309%7D -- 3.1 Кб -- 10.04.2016
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2611. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BFB4C868E-684A-47DB-8F0C-AE88DAFC2A6D%7D
. This photograph of the Sun, taken by the Atmospheric Imaging Assembly instrument on NASA's Solar Dynamics Observatory, shows how image processing techniques developed at SAO can reveal the faint, inner corona. At the Sun's limb, prominences larger than Earth arc into space. Bright active regions like the one on the Sun's face at lower center are often the source of huge eruptions known as coronal mass ejections. NASA/LMSAL/SAO
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BFB4C868E-684A-47DB-8F0C-AE88DAFC2A6D%7D -- 3.6 Кб -- 10.04.2016
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2612. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BFACF39E2-F0AE-4832-9F95-E2A420D14506%7D
. Researchers based at Princeton University, the California Institute of Technology, and Ashima Research suggest that Mars' roughly 3.5-mile high (5.6 kilometers) Mount Sharp most likely emerged as strong winds carried dust and sand into Gale Crater where the mound sits. If correct, the research could dilute expectations that the mound is the remnant of a massive lake, which would have important implications for understanding Mars' past habitability. // NASA/JPL-Caltech/MSSS
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BFACF39E2-F0AE-4832-9F95-E2A420D14506%7D -- 3.8 Кб -- 10.04.2016
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2613. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BF5438634-12F9-46C8-B32E-C8E02D92EC7A%7D
. Luis Argerich from Buenos Aires, Argentina, captured Comet PANSTARRS in the sky above Mercedes, Argentina, on February 11, 2013. The comet shone at magnitude 4.5 to the left of an Iridium flare.
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BF5438634-12F9-46C8-B32E-C8E02D92EC7A%7D -- 3.1 Кб -- 10.04.2016
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2614. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BE8096472-8553-4964-919B-0E357C0A2985%7D
. ATLAS project head John Tonry with a conceptual drawing for an ATLAS telescope. The project would use two of these 20-inch telescopes. // UH/IfA
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BE8096472-8553-4964-919B-0E357C0A2985%7D -- 3.0 Кб -- 10.04.2016
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2615. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BDD253D4C-6832-4A48-BEDF-F843D98DB7A1%7D
. Images from Swift's Ultraviolet/Optical (white, purple) and X-ray telescopes (yellow and red) were combined in this view of GRB 110328A. The blast was detected only in X-rays, which were collected over a 3.4-hour period on March 28. NASA/Swift/Stefan Immler
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BDD253D4C-6832-4A48-BEDF-F843D98DB7A1%7D -- 3.2 Кб -- 10.04.2016
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2616. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BC8CD6F24-6408-45A9-B002-15F6EB524070%7D
. NASA's Chandra X-ray Observatory completed this four-hour exposure of GRB 110328A on April 4. The center of the X-ray source corresponds to the very center of the host galaxy imaged by Hubble (red cross). NASA/CXC/ Warwick/A. Levan
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BC8CD6F24-6408-45A9-B002-15F6EB524070%7D -- 3.2 Кб -- 10.04.2016
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2617. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BC5C37E6E-09AA-4D29-ABFF-3678A59AF303%7D
. This diagram compares our own solar system to Kepler-47, a double-star system containing two planets, one orbiting in the so-called "habitable zone." // Credit: NASA/JPL-Caltech/T. Pyle
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BC5C37E6E-09AA-4D29-ABFF-3678A59AF303%7D -- 3.1 Кб -- 10.04.2016
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2618. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BB82C0F2D-BC07-462B-B569-3EE6456CD747%7D
. The Egg Nebula. Credit: ESA/Hubble, NASA
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BB82C0F2D-BC07-462B-B569-3EE6456CD747%7D -- 2.7 Кб -- 10.04.2016
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2619. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BB42005DF-EAF2-4359-9A0D-D9987CE5310A%7D
This plot shows the projected motion of the red dwarf star Proxima Centauri (green line) over the next decade, as plotted from Hubble Space Telescope observations. ... Because Proxima Centauri is the closest star to our Sun, its angular motion across the sky is relatively fast compared to much more distant background stars. This means that in 2014 and 2016 Proxima Centauri will pass in front of two background stars that are along its path. ...
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BB42005DF-EAF2-4359-9A0D-D9987CE5310A%7D -- 4.6 Кб -- 10.04.2016
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2620. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BA8B86F8E-A84A-4582-9444-4E33AA799FF9%7D
. This is a visible-light image of GRB 110328A's host galaxy (arrow) taken April 4 by the Hubble Space Telescope's Wide Field Camera 3. The galaxy is 3.8 billion light-years away. NASA/ESA/A. Fruchter (STScI)
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BA8B86F8E-A84A-4582-9444-4E33AA799FF9%7D -- 3.1 Кб -- 10.04.2016
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