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Moon ¤ë²y (11/9/2003)
¤£ª¾¹D¬O§_¤¤¬î¸`ªºÃö«Y¡A¤j®a³£·|¥H¬°¤K¤ë¤Q¤­ªº¤ë¥ú¬O³Ì¶ê³Ìè°ªº¡A¦ý¤@¦~¦³«Ü¦h¦¸º¡¤ë¡Aµ´¤£·|¤ñ¤¤¬îªº»¹¦â¡CµM¦Ó¡A¤µ¤é±a¤j®a¥h¤ë²y¤W¨«¤@½ë¡A¬Ý¬Ý¥­®É§Ú­Ì¬Ý¤£¨ìªº¦a¤è¡A³oùجO¤ë²yªº«nÃä¡A¨ä¤¤¤@¨Ç¦a¤èªø´Á­IµÛ¦a²y¡A§Ú­Ì¦b¦a²y¤W«ÜÃø©ÎªÌ¤°¦Ü¥Ã»·¤]¤£¯à¨£¨ì¥¦­Ì¡C¥k¤è¶Â¦âªº¬O¥vÁÚ¥q®ü¡A¥ªÃ䤤¶¡ªº¬O¬x«O±oÀô§Î¤s¡A¦Ó¦b¥vÁÚ¥q®ü¤§¤U¡A¥Ñ¥k¦Ü¥ªªº¬OÀô§Î¤s¥­¤s¡B´µ¥iù¦h¤Ò´µ¥d(§Y©~§¤Ò¤H)¡B©~§(©~§¤Ò¤Hªº¤V¤Ò)¡A¥L­Ì¦b¤ë²y¤W¤]¬O¤@°_¡A¥i¨£Àô§Î¤sªº©R¦W¤£¬O­J¨Óªº¡C

Caption:: Leaving the scene of their explorations, the Apollo 15 astronauts photograph the Moon's southern hemisphere shortly after firing their rocket engine to begin the trip back to Earth. The image includes a portion of the lunar farside, which is not visible from Earth. Mare Smythii to the right, Humboldt Crater at the central left, whereas Craters Hirayama, Sklodowska, Curie are along the bottom from the right to left. This view was captured by a high-resolution camera stored in the side of the service module.

Credit:: Alfred Worden, Project Full Moon

Aurora over Clouds ¶³¤W·¥¥ú (10/9/2003)
¤]¤£¬O²Ä¤@¦¸µ¹¤j®a¬Ý·¥¥ú¬Û¤F¡A¤µ¦¸ªº·¥¥úµL¤§«e¨â±i¨º»ò©_§Î©Çª¬¡A¦ý§A¥i¥H¬Ý¨ì·¥¥ú©M¶³¤@°_¡A¦Ó¥B°ª©ó¶³¼h¤W¡C³o¥¿¬O·¥¥ú§Î¦¨©ó¤j®ð¼hªº³»³¡¡A»·»·°ª¹L¸û§Cªº¶³¼h¡C¥k­±¨º­Ó«Ü¥ú«Gªº¬O¤ë«G¡A¦Ó´ò¤W¤]¦³µÛ¥¦ªº­Ë¼v¡C

Caption:: Aurorae usually occur high above the clouds. The auroral glow is created when fast-moving particles ejected from the Sun impact air molecules high in the Earth's atmosphere. An oxygen molecule, for example, will glow in a green light when reacquiring an electron lost during a collision with a solar particle. The lowest part of an aurora will typically occur at 100 kilometers up, while most clouds usually exist only below about 10 kilometers. The relative heights of clouds and auroras are shown clearly in the above picture taken last month from near Quebec City, Canada. The most likely time to see an aurora is around midnight.

Credit:: Dominic Cantin

Saturn II ¤g¬P II (9/9/2003)
³Ì¬°¤H¼ô±xªº¦æ¬P¡A¤@©w¬O¤g¬P¤F¡A¥þ¦]¬°¬O¥¦¨º¯S§OÅã²´ªºÀô¡C¦ý§Ú·Q¤£¬O«Ü¦h¤H·|ª¾¹D¡A³o­Ó¤g¬PÀô¬O·|ÅܤjÅܤpªº¡A©ÎªÌ§ÚÀ³¸Ó»¡²M·¡¡A¬O¤g¬P¬Ý¤W¥hªº¨¤«×·|§ïÅÜ¡A¦Ó¨Ï§Ú­Ì¬Ý¤W¥h¤g¬P®É¡A¬Ý¨ìªº¤g¬PÀô·|ÅܤjÅܤp¡C³o¬O«¢«k¤ÓªÅ±æ»·Ã誺·s¬Û¡A³o®Éªº¤g¬P¥¿³B©ó¤g¬PÀô³Ì¶É±×ªº®É­Ô¡A¤]¬O¬Ý«n·¥©MÀôªº«nºÝ³Ì²M·¡ªº®É­Ô¡C¦ý³o±i¬Û¬O©çÄáµµ¥~½uªi¬qªº¡A©Ò¥H¬Ý¤W¥hªºÃC¦â¸ò´¶³qªº¦³©Ò¤£¦P¡C

Caption:: This is one of the series of images of Saturn, as seen at many different wavelengths, this one is obtained by UV, when the planet's rings were at their maximum tilt of 27 degrees toward Earth. Saturn experiences seasonal tilts away from and toward the Sun, much the same way Earth does. This happens over the course of its 29.5-year orbit. This means that approximately every 30 years, Earth observers can catch their best glimpse of Saturn's South Pole and the southern side of the planet's rings. Between March and April 2003, researchers took full advantage to study the gas giant at maximum tilt. They used NASA's Hubble Space Telescope to capture detailed images of Saturn's Southern Hemisphere and the southern face of its rings.

Credit:: NASA and E. Karkoschka (University of Arizona)

Abell 1689 (8/9/2003)
¤£ª¾¹D¤j®a¦³¨S¦³¬Ý¹L³o¤@Ãþªº¬Û¡A¦t©z²`³Bªº¬Û¡C·í§Ú­Ì±æ¦V¦t©zªº²`³Bªº®É­Ô¡A¥u·|¨£¨ì¤@¤ù¶Â·t¡A¤°»ò¤]¬Ý¤£¨ì¡A³o¤]¸ò§Ú­Ì¦×²´¬Ý¨ìªºªF¦è¦³­­¦³Ãö¡A¤Ó·tªº§Ú­Ìªº²´·ú®Ú¥»¬Ý¤£¨£¡A¤]¥u¦³¾a»ö¾¹ªºÀ°§U¡A¤~¥i¥H¬Ý¨ì«Ü»·«Ü·tªº¦t©z²`³B¡C¦ý¦t©zªº²`³B¤]¤£¤@©w¦h«º¦h±m¡A¸I¥©§A¹J¤W­«¤O³zÃ誺²{¶H¡A¤~·|¬Ý¨ì¹Ï¤¤ªº¹Òªp¡C¥Ñ«¢«k¤ÓªÅ±æ»·Ãè©ç¦^¨Óªº¬P¨t¹ÎAbell 1689¡A¦]¬°«e­±¦³¤@¨Ç¬Ý¤£¨£ªºª«½è¥O¥ú½u§ïÅܤè¦V¡A©Ò¥H¥O¬Ý¨ìªºµ{²{¦h­«¼v¹³¡A³o¬O­«¤O³zÃ誺­ì²z¡C³o±i¬Û¤ñ¤§«e¥ô¦ó¤@±iªº³zÃè¬Û³£­n²M·¡¡A«Ü¦h²Ó·Lªº¦a¤è³£¬Ý±o¦n²M·¡©O¡C

Caption:: The Advanced Camera for Surveys (ACS) aboard NASA's Hubble Space Telescope has used a natural "zoom lens" in space to boost its view of the distant universe. Besides offering an unprecedented and dramatic new view of the cosmos, the results promise to shed light on galaxy evolution and dark matter in space. Hubble peered straight through the center of one of the most massive galaxy clusters known, called Abell 1689. For this observation, Hubble had to gaze at the distant cluster, located 2.2 billion light-years away, for more than 13 hours. The gravity of the cluster's trillion stars ¡X plus dark matter ¡X acts as a 2-million-light-year-wide "lens" in space. This "gravitational lens" bends and magnifies the light of galaxies located far behind it, distorting their shapes and creating multiple images of individual galaxies.

Credit:: NASA, N. Benitez (JHU), T. Broadhurst (The Hebrew University), H. Ford (JHU), M. Clampin(STScI), G. Hartig (STScI), G. Illingworth (UCO/Lick Observatory), the ACS Science Team and ESA

Japanese Macaques ¤é¥»ônµU (7/9/2003)
³B©ó·¥§Nªº¤é¥»¥_®ü¹D¡A¤é¥»ônµU(¤]ºÙ³·µU)¬O¤HÃþ¥H¥~©~©ó³Ì¥_ªºÆFªøÃþ°Êª«¡C¨e­Ì«ÜÁo©ú¡AÀ´±o§Q¥Î·í¦aªº¤ÑµM¸ê·½¡Ð·Å¬u¨Ó«O«ùÅé·Å¡A¨e­Ì®É±`³£¤T¤­¤@°_¨«¨É¨ü·Å¬u¡A¯uÀ´¨É¨ü¡I

Caption:: It may be called the Jigokudani Wild Monkey Park, but the Japanese macaques here have taken up one of life's more civilized pleasures: hot tubbing. A series of hot springs help keep the monkeys warm through the cold winters. Also known as snow monkeys, Japanese macaques are the world's northernmost non-human primates.

Credit:: Tim Laman


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