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701. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B1B3D24C1-BA4A-4C3B-8DA1-94B2EA747663%7D
How much would you weigh on another star? ... If stars had solid surfaces on which you could stand, then your weight would change from star to star. Here we show how much a 75-kilogram (165 pounds) adult would tip the bathroom scale in the surface gravities of three stars. ... You'd weigh 20 times more than on Earth. A red giant star (the far-future fate of our Sun, with a diameter about 35 times larger) has a much weaker pull at its surface, so you'd be 50 times lighter. ...
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B1B3D24C1-BA4A-4C3B-8DA1-94B2EA747663%7D -- 4.3 Кб -- 10.04.2016
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702. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BE012675E-A1D5-4235-90AF-9F6580295919%7D
. Artist s concept of NASA s New Horizons spacecraft as it passes Pluto and Pluto s largest moon, Charon, in July 2015. NASA/JHU APL/SwRI/Steve Gribben
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BE012675E-A1D5-4235-90AF-9F6580295919%7D -- 3.1 Кб -- 10.04.2016
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703. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BAFCA0A33-BDF3-4F4D-BE18-F6CBE8A062E0%7D
. The intense gravity fields of two black holes merge in a computer simulation . performed by scientists at NASA s Goddard Space Flight Center in Greenbelt, Maryland. Astronomers hope to detect gravity waves emitted during black-hole mergers. Christopher Henze/NASA Ames Research Center
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BAFCA0A33-BDF3-4F4D-BE18-F6CBE8A062E0%7D -- 3.4 Кб -- 10.04.2016
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704. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BA218E296-B268-4190-B265-6B6280764FEB%7D
. NASA, ESA, PSI, JHU/APL, STScI/AURA
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BA218E296-B268-4190-B265-6B6280764FEB%7D -- 2.8 Кб -- 10.04.2016
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705. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B5941FDE3-A1E0-4B01-9D8F-ED48B82BB6D3%7D
Gravitational waves from inflation generate a faint but distinctive twisting pattern in the polarization of the cosmic microwave background (CMB), known as a "curl" or B-mode pattern. ... Shown here is the actual B-mode pattern observed with the BICEP2 telescope, with the line segments showing the polarization from different spots on the sky. The red and blue shading shows the degree of clockwise and anti-clockwise twisting of this B-mode pattern. BICEP2 Collaboration ...
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B5941FDE3-A1E0-4B01-9D8F-ED48B82BB6D3%7D -- 4.1 Кб -- 10.04.2016
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706. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B58FF67B3-940E-4D5E-BA68-D2760FA44B96%7D
Pluto and Charon, the largest of Pluto's five known moons, seen January 25 (left) and 27 (right), 2015, through the telescopic Long-Range Reconnaissance Imager (LORRI) on NASA's New Horizons spacecraft. New Horizons was about 126 million miles (203 million kilometers) from Pluto when the frames to make the first image were taken and about 1.5 million miles (2.5 million kilometers) closer for the second set. ...
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B58FF67B3-940E-4D5E-BA68-D2760FA44B96%7D -- 4.9 Кб -- 10.04.2016
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[ Сохраненная копия ] Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BCE59C370-CA6E-4317-A962-6F2594602774%7D -- 4.9 Кб -- 10.04.2016
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707. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B1715B4C3-B4A1-4769-B574-4FAC1B0E11BA%7D
. Within a cloud of hot gas, radio-energy jets emanate from two supermassive black holes (the two bright spots) in the galaxy NGC 1128. Recent observations suggest the black holes will merge into one, radiating a cosmic earthquake of gravitational waves. X-ray imagery: NASA/CXC/AIFA/D. Hudson T. Reiprich et al.; Radio imagery: NRAO/VLA/NRL
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B1715B4C3-B4A1-4769-B574-4FAC1B0E11BA%7D -- 3.5 Кб -- 10.04.2016
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708. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B1701020D-62FA-42D5-B0EA-181FEAAC54E2%7D
The Pictor A galaxy has a supermassive black hole at its center, and material falling onto the black hole is driving an enormous beam, or jet, of particles at nearly the speed of light into intergalactic space. These images show X-ray data obtained by Chandra at various times over 15 years and radio data from the Australia Telescope Compact Array. ... X-ray: NASA/CXC/Univ of Hertfordshire/M.Hardcastle et al., Radio: CSIRO/ATNF/ATCA ...
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B1701020D-62FA-42D5-B0EA-181FEAAC54E2%7D -- 4.1 Кб -- 10.04.2016
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709. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BE4CDAAC8-642D-4430-8A0D-7B510139FC73%7D
. This image of Pluto and its largest moon, Charon, was taken by the Ralph color imager aboard New Horizons on April 9, 2015, from a distance of about 71 million miles (115 million kilometers). It is the first color image ever made of the Pluto system by a spacecraft on approach. NASA/Johns Hopkins University Applied Physics Laboratory/Southwest Research Institute
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BE4CDAAC8-642D-4430-8A0D-7B510139FC73%7D -- 3.5 Кб -- 10.04.2016
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710. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BDDDA27A5-ADCD-4E20-9D3D-48EB656F446D%7D
. These two galaxy clusters are part of the "Frontier Fields" project that obtains long observations with multiple telescopes. X-ray: NASA/CXC/SAO/G.Ogrean et al.; Optical: NASA/STScI; Radio: NRAO/AUI/NSF
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BDDDA27A5-ADCD-4E20-9D3D-48EB656F446D%7D -- 3.2 Кб -- 10.04.2016
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711. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BAA2BF042-82E2-49BD-B02D-2C23657E1381%7D
. This artist s impression shows how photons in the cosmic microwave background (CMB) are deflected by the gravitational lensing effect of massive cosmic structures as they travel across the universe. Gravitational lensing creates tiny, additional distortions to the mottled pattern of the CMB temperature fluctuations. A small fraction of the CMB is polarized; one component of this polarized light, B-modes, have been given an additional signature by gravitational lensing. ESA/Planck Collaboration
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BAA2BF042-82E2-49BD-B02D-2C23657E1381%7D -- 3.9 Кб -- 10.04.2016
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712. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B9549CB5C-7EF3-48E9-956F-3996658EE83E%7D
. This is a composite image showing the visible and near infrared light spectrum collected from Hubble's ACS and WFC3 instruments over a nine-year period. NASA/ESA/H. Teplitz and M. Rafelski (IPAC/Caltech)/A. Koekemoer (STScI)/R. Windhorst (Arizona State Univ.)/Z. Levay (STScI)
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B9549CB5C-7EF3-48E9-956F-3996658EE83E%7D -- 3.3 Кб -- 10.04.2016
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713. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B5BE01890-DB20-44D6-AD57-B9CEB1A4DC8B%7D
. The close encounter between Comet Siding Spring and Mars flooded the planet with an invisible tide of charged particles from the comet's coma. The dense inner coma reached the surface of the planet, or nearly so. The comet's powerful magnetic field temporarily merged with, and overwhelmed, the planet's weak field, as shown in this artist's depiction. NASA/Goddard
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B5BE01890-DB20-44D6-AD57-B9CEB1A4DC8B%7D -- 3.5 Кб -- 10.04.2016
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714. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B510CE4E4-88A1-442B-8AC7-696CEB660213%7D
. This visualization of Planck data portrays the interaction between interstellar dust in the Milky Way and the structure of our Galaxy s magnetic field. The color scale represents the total intensity of dust emission, revealing the structure of interstellar clouds in the Milky Way. The texture is based on measurements of the direction of the polarized light emitted by the dust, which in turn indicates the orientation of the magnetic field. ESA/Planck Collaboration
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B510CE4E4-88A1-442B-8AC7-696CEB660213%7D -- 3.8 Кб -- 10.04.2016
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715. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B47098038-EB87-4E85-B546-B53A2D3AE6CE%7D
The highlighted region of this area of Planck data shows the position of a small patch of the sky that was observed with two ground-based experiments at the South Pole, BICEP2 and the Keck Array, and yielded a possible detection of curly B-modes in the polarization of the cosmic microwave background (CMB), the most ancient light in the history of the universe. ... ESA/Planck Collaboration ...
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B47098038-EB87-4E85-B546-B53A2D3AE6CE%7D -- 4.1 Кб -- 10.04.2016
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716. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B368663D3-1B92-465D-B002-4757CAAD050F%7D
. Timeline of the universe . NASA/WMAP Science Team
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B368663D3-1B92-465D-B002-4757CAAD050F%7D -- 2.8 Кб -- 10.04.2016
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717. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BF93C9DDF-0D3B-4CA5-AFDF-628D466373D8%7D
. An artist s concept of the distribution of the ambient gas around IRAS 16547-4247. The central high-density gas cloud is thought to contain multiple high-density protostars. Two outflows of gas spurt from the central part in the vertical and horizontal directions, respectively, while pushing the ambient gas away, which makes a balloon-like structure. A pair of narrow jets is the one that was found in past observations. NAOJ
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BF93C9DDF-0D3B-4CA5-AFDF-628D466373D8%7D -- 3.7 Кб -- 10.04.2016
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718. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B952034DB-BEC1-4CF4-9C36-20D4AFC0FD04%7D
. Astronomers using the Atacama Large Millimeter/sub-millimeter Array have imaged the episodic outflow of a young protostar known as CARMA-7. The twin jets each nearly 1.5 trillion kilometers long have distinct gaps, revealing that the star is growing by fits and starts. B. Saxton, NRAO/AUI/NSF; A Plunkett et al.; ALMA, NRAO/ESO/NAOJ
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B952034DB-BEC1-4CF4-9C36-20D4AFC0FD04%7D -- 3.5 Кб -- 10.04.2016
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719. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B565A930E-BD11-4E77-91D4-2FFE4D874B63%7D
. The Twin Jet Nebula (PN M2-9) is a striking example of a bipolar planetary nebula. Bipolar planetary nebulae are formed when the central object is not a single star but a binary system. Studies have shown that the nebula s size increases with time, and measurements of this rate of increase suggest that the stellar outburst that formed the lobes occurred just 1,200 years ago. ESA/Hubble NASA; Acknowledgement: Judy Schmidt
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B565A930E-BD11-4E77-91D4-2FFE4D874B63%7D -- 3.7 Кб -- 10.04.2016
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720. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B2A802332-7348-4B9D-9AF4-0AF36F4B7D25%7D
. An artist s impression of some of the first stars in the early universe. Five protostars are seen here forming in the center of disks of gas. Shantanu Basu, University of Western Ontario
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B2A802332-7348-4B9D-9AF4-0AF36F4B7D25%7D -- 3.2 Кб -- 10.04.2016
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