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http://www.iki.rssi.ru/solar/eng/gaspra.htm.
http://www.iki.rssi.ru/solar/eng/gaspra.htm.
1. Asteroid Gaspra
Gaspra . ... On October 29, 1991, Galileo came within 1,600 kilometers (1,000 miles) of Gaspra. ... These two color views of the asteroid Gaspra were produced by combining three images taken through violet, green, and infrared filters by the Galileo spacecraft on October 29, 1991, from a distance of about 16,000 kilometers (10,000 miles). ... The earliest view (upper left) was taken 5 hours, 45 minutes before closest approach when the spacecraft was 164,000 kilometers (102,000 miles) from Gaspra. ...
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Ссылки http://www.iki.rssi.ru/solar/eng/gaspra.htm -- 8.4 Кб -- 15.10.1997
[ Сохраненная копия ] Ссылки http://www.arcetri.astro.it/irlab/Astro/solar/eng/gaspra.htm -- 9.3 Кб -- 15.03.1998
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[ Сохраненная копия ] Ссылки http://www.arcetri.astro.it/irlab/Astro/solar/eng/gaspra.htm -- 9.3 Кб -- 15.03.1998
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2. XWare > APOD
Astronomy Picture of the Day . Asteroid 1998 WT24 Passes Near Earth . ... Last week, an asteroid approached unusually close to the Earth. ... Pictured above, the kilometer-sized asteroid was imaged crossing the sky on December 14, two days before closest approach. ... Hot blue stars, red glowing hydrogen gas, and dark, obscuring dust clouds are strewn through this dramatic region of the Milky Way in the southern constellation of Ara (the Altar). ... Finding Dark Matter . ... Where is dark matter? ...
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Ссылки http://www.astronet.ru/db/xware/apod.html?page=96&d=2004-07 -- 15.5 Кб -- 12.04.2016
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3. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B34CF81E9-E017-4329-AAD5-ADF51793AD2D%7D
. This set of images from the radar instrument on NASA's Cassini spacecraft shows a relatively "fresh" crater called Sinlap (left) and an extremely degraded crater called Soi (right). Sinlap has a depth-to-diameter ratio close to what we see on Jupiter's moon Ganymede. Soi has a shallow depth compared to similar craters on Ganymede. These craters are both about 50 miles (80 kilometers) in diameter. // Credit: NASA/JPL-Caltech/ASI/GSFC
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Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B34CF81E9-E017-4329-AAD5-ADF51793AD2D%7D -- 3.7 Кб -- 10.04.2016
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4. First Observation of a Close Earth-Approaching Near-Earth Asteroid Using the
... Figure 8: Can you detect the motion of the near-Earth asteroid 2000PH against the background stars during its close approach to Earth around 27 July 2004? ... Down) observed and imaged the unusual near-Earth asteroid 2000PH during its close approach to the Earth around 27 July 2004. The observations were carried out remotely using the new 2m aperture Faulkes telescope situated on the 10,000-foot summit of Haleakala, on the island of Maui in Hawaii. ...
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Ссылки http://star.arm.ac.uk/annrep/annrep2004/node65.html -- 7.5 Кб -- 19.04.2005
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5. The Orion OB1 Association
... Early studies of PMS stars focused on T associations, especially Taurus-Auriga. However, one might expect low mass star formation to be different in OB associations. ... He identified Orion OB1a as the stars northwest of the belt. Orion OB1b is composed of the stars near the belt, including the belt stars and Orionis. ... He finds no perceptible distance change within the Orion OB1b association and finds the distance modulus to be 7.8 and 7.9 for Orion OB1a and OB1b respectively. ...
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Ссылки http://hea-www.harvard.edu/~swolk/thesis/optical/node2.html -- 5.3 Кб -- 02.10.2012
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6. APOD: 2000 October 27 - Close To Eros
... Each day a different image or photograph of our fascinating universe is featured, along with a brief explanation written by a professional astronomer. 2000 October 27 . Close To Eros . Credit: NEAR Project , JHU APL , NASA . Explanation: Scroll right and fly close over asteroid Eros! ... The car-sized Near Shoemaker spacecraft is now on its way to a higher, more stable orbit about 200 kilometers above asteroid Eros . ... About APOD | ... NASA Technical Rep.: ...
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Ссылки http://www.sai.msu.su/apod/ap001027.html -- 4.5 Кб -- 01.10.2012
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7. Lunar Drawings
Crater Gassendi . ... I made this drawing was made on the 26th of november 2001. If you compare this one with the previous drawing of Gassendi (below) the differences are clear. ... This drawing was made on the 28th of september 2001. After nearly a full month without observations I had a one hour gap between the thicker clouds. ... This drawing was made on the 29th of august 2001. ... This drawing was made on the 27th of august 2001. ... This drawing was made on the 25th of august 2001. ...
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Ссылки http://aberrator.astronomy.net/moon/index.html -- 13.5 Кб -- 28.11.2001
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8. Terrestrial Silicates Compared to Astronomical Silicates
The silicates that produce the 10 and 18 micron features appear to be broadly similar to terrestrial minerals such as Forsterite and Enstatite. ... Where pre-solar silicate dust grains can be isolated from meteorite material, these also tend to be Mg-rich silicates rather than Fe-rich silicates. ... It has been suggested that the interstellar silicate grains have a different 10 micron feature profile than what is observed for the silicates around evolved stars. ...
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Ссылки http://www.stsci.edu/~volk/features1a.html -- 7.8 Кб -- 27.05.2014
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9. Kepler 36b and c: Too Close for Comfort | Astronotes
... Planets . ... Earth Satellites . ... Looking in the direction of the constellation Cygnus the Swan and launched by NASA in 2009 is the Kepler Space Observatory.Many previous missions searching for exoplanets mainly detected large giant planets, like large hot Jupiters (it is easier to detect larger planets).However KeplerтАЩs main objective is to search for much smaller planets located in a habitable zone which is not too close nor too far from their star; planets which may be just like our Earth. ...
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Ссылки http://www.armaghplanet.com/blog/too-close-for-comfort.html -- 46.3 Кб -- 09.04.2016
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10. http://www.naic.edu/~phil/430yagi/cross_01aug06.html
... compare the system performance of 01aug06 and may06 (.ps) ( .pdf ) The 430 Mhz yagi antenna was moved closer to the line feed around 25jul06. ... This was the same source that was used on 29may06. 12 crosses were done with the yagi and 3 crosses with the linefeed. ... Each strip was rotated by the measured pointing error before averaging. ... The average yagi pointing errors are 3.56 Amin az and -.92 amin za. ... These pointing errors say the offsets should have been: az: .809, za: -.9453 deg. ...
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Ссылки http://www.naic.edu/~phil/430yagi/cross_01aug06.html -- 8.6 Кб -- 12.08.2006
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11. АСТРОКУРЬЕР, НОВОГОДНИЙ ВЫПУСК 1 января 2000 г.
КОСМИЧЕСКИЙ КАЛЕНДАРЬ ЯНВАРЯ 2000 ГОДА . ... Jan 01 - Year 2000 . Jan ?? ... Jan 01 - Asteroid 1996 AX1 Closest Approach To Earth (0.702 AU) . ... Jan 03 - Asteroid 3745 Petaev Closest Approach To Earth (1.862 AU) . ... Jan 05 - Asteroid 1999 VO11 Near-Earth Flyby (0.218 AU) . ... Jan 08 - Comet P/1998 VS24 (LINEAR) Closest Approach To Earth (2.915 AU) . ... Jan 12 -[Image][Dec 02] Asteroid 1999 WA2 Closest Approach To Earth (1.100 AU) . ... Jan 14 - Mercury Occults 53 Sgr (6.9 Magnitude Star) . ...
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Ссылки http://astrocourier.chat.ru/2000/20jan/20jan5.htm -- 13.7 Кб -- 09.04.2016
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12. Pulkovo NEO Page: Apparent Close Approaches to the Stars
. Pulkovo NEO Page . Central Astronomical Observatory at Pulkovo . of Russian Academy of Sciences, St.-Petersburg, Russia . Apparent Close Approaches of Near-Earth Asteroids to the Stars for April 2016 . By these observations it is possible to obtain the positions of asteroids with higher accuracy. This page includes the ephemerides of such phenomena for some observatories, namely: . Pulkovo . CrAO . Kourovskaya . Majdanak . Pulkovo Obs. Mountain Station . Mondy .
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Ссылки http://www.gao.spb.ru/personal/neo/eng/approach/main.htm -- 9.9 Кб -- 28.03.2016
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13. Phil Plait's Bad Astronomy: Bitesize Astronomy
... Bad Astronomy . ... Bitesize Astronomy . ... Bad Astro Store . ... Site Info . ... It is from from Voyager 1 and shows a whopping big impact crater dominating the profile of the moon. Note that Mimas is about 400 kilometers across (about 250 miles). ... The wall around the crater is 5 kilometers high, and that central peak rises 6 kilometers above the surface (many impact craters have a large central peak which is caused by a pressure rebound from the impact). ... 2008 Phil Plait. ...
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Ссылки http://www.badastronomy.com/bitesize/mimas.html -- 19.9 Кб -- 09.04.2016
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14. http://selena.sai.msu.ru/Symposium/lipskiy.pdf
LIPSKIY-RODIONOVA' LUNAR ANTIPODES AS PRECURSORS OF A REGULAR WAVE PLANETOLOGY G.G.Kochemasov IGEM of the Russian Academy of Sciences, Moscow, Russia kochem@igem.ru / Fax: (009)(095)230 21 79 The first observations of the lunar far side allowed to compare it with the near side and draw very important conclusions in the very beginning of planetary studies based on spacecrafts. ... Celestial bodies are dichotomic. ... The concept of celestial bodies includes Sun (a star) as one of them. ...
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Ссылки http://selena.sai.msu.ru/Symposium/lipskiy.pdf -- 117.1 Кб -- 06.10.2008
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15. Artist's impression of the asteroid Lutetia making a close approach to a planet
.
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Ссылки http://www.eso.org/public/images/eso1144b/zoomable/ -- 1.9 Кб -- 12.04.2016
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16. http://www.ipa.nw.ru/conference/2002/sovet/PS/KISELEVA.PS
... 8, ``Celestial Mechanics'', 2002 CCD observations of planetary satellites and occultations and close approachments of stars by asteroids with 26 inch refractor of Pulkovo observatory T. P. Kiseleva, I. S. Izmailov, M. A. Mozhaev Pulkovo Observatory, St. Petersburg, Russia ST--6 CCD camera has been used with 26-- inch Refractor at Pulkovo for ob servations of ... These estimates are \Sigma0:015 arcsec and \Sigma0:014 arcsec for X and Y correspondingly. ...
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Ссылки http://www.ipa.nw.ru/conference/2002/sovet/PS/KISELEVA.PS -- 32.8 Кб -- 19.08.2002
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17. casacore: casa/Utilities/Compare.h Source File
... Classes . Files . ... File List . File Members . casa . Utilities . ... National Radio Astronomy Observatory 00023 //# 520 Edgemont Road 00024 //# Charlottesville, VA 22903-2475 USA 00025 //# 00026 //# $Id: Compare.h 20551 2009-03-25 00:11:33Z Malte.Marquarding $ 00027 00028 #ifndef CASA _COMPARE_H 00029 #define CASA _COMPARE_H 00030 00031 //# Includes 00032 #include casa /aips.h 00033 #include casa / Utilities /DataType.h 00034 00035 namespace casa { //# NAMESPACE ...
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Ссылки http://www.atnf.csiro.au/computing/software/casacore/casacore-1.2.0/doc/html/Compare_8h_source.html -- 15.0 Кб -- 14.02.2011
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18. Jupiter Moon Callisto
... Impact craters and associated concentric rings are about the only features to be found on Callisto. ... It has a bright central region that is 600 kilometers in diameter, and its rings extend to 3000 kilometers in diameter. ... This image shows the heavily cratered surface of Callisto. ... Also visible is a fresh, sharp-rimmed crater some 90 km (56 miles) across named Igaluk (center left third of picture), and a bright zone in the south polar area (bottom of image) which could be an impact scar. ...
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Ссылки http://www.iki.rssi.ru/solar/eng/callisto.htm -- 13.8 Кб -- 15.10.1997
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19. Amateur Astronomers Association of New York ? Amateur Astronomers Association
... Observing . ... Solar Observing . ... April 3 (SUN) - Solar Observing, Central Park , Manhattan . ... APRIL'S SKY . ... Lecture Series at the American Museum of Natural History The Amateur Astronomers Association is proud to present an astronomy lecture series from October through May each year for our members and the .. ... The€аAmateur Astronomers Association of New York€аwas organized in 1927 to promote the study of Astronomy, emphasizing its cultural and inspirational value. ...
20. ASP: Miranda: A Jigsaw Puzzle World
... When the Voyager 2 spacecraft flew by the planet Uranus in January 1986, astronomers were treated to their first close-up glimpse of the satellites that orbit the seventh planet. ... But by far the most intriguing of those 15 satellites was a jigsaw-puzzle world called Miranda . ... How dark was it at Miranda? One of the Voyager scientists put it this way: Taking pictures in the Uranus system is like trying to do photography in a ballpark at night when the only light comes from a single candle. ...
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Ссылки http://www.astrosociety.org/edu/publications/tnl/07/07.html -- 12.0 Кб -- 02.10.2012
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