<<Next PAGE 5:: Previous>>

Earth from Mars ±q¤õ¬P¬Ý¦a²y (24/5/2003)
¤ÓªÅ¡A¬O¤@­Ó«Ü¼sÁ諸¦a¤è¡A¤j±o§A·Q¹³¤£¨ì¡A¨C¤@¼Ëª«¥ó¦b¦t©z¤¤³£²Ó¤p±o¤£¯à§Î®e¡C¦a²y¦b¦t©z¤¤¡A¥u¬O¤@­Ó«Ü¤p«Ü¤pªºÂÅÂI¡A°ò¥»¤W¥X¤F¤Ó¶§¨t´N·|³s¦a²y³£¬Ý¤£¨£¤F¡A¥i·Q¦Óª¾¡A§Ú­Ì¦³¦h²Ó¤p¡C¦b¤j®ð¼h¤W¬Ý¦^¦a²yªº¬Û´N¨£±o¦h¤F¡A¥Ñ¤õ¬P¡]¥Ñ¤õ¬P¥þ²y°É´úªÌ¸¹¤ÓªÅ²î©çªº¡^±æ¦^¦a²yªº¬Û­Ë¬O²Ä¤@¦¸¡A§A¿ì»{¨ì³o¬O¦a²yªº¬Æ»ò¦a¤è¶Ü¡H·Qª¾µª®×ªº¸Ü¡A½Ð¬Ý­^¤åªº¸Ñ»¡¡C¥k¤W¨¤ªº¬O¤°»ò¡H·íµM¬O¤ë²y¡A¤£­n§i¶D§Ú§A¤£ª¾¹D§r¡A­ì¨Ó¤ë²y¬Û¹ï©ó¦a²y¨Ó»¡¡A¤@ÂI¤]¤£ºâ²Ó¤p¡C¯u¬O¶V¬Ý´N¶V³ßÅw³o±i¬Û¡A±N¨Ó­YªG¤HÃþ²¾¨ì¤õ¬Pªº¸Ü¡A±æ¤W¤ÓªÅ¡A¦^¬Ý¦Û¤vªº¦Ñ®a®É¡A´N¬O³o­Ó¼Ë¤l¤F¡C

Caption:: This is the first image of Earth ever taken from another planet that actually shows our home as a planetary disk. Because Earth and the Moon are closer to the Sun than Mars, they exhibit phases, just as the Moon, Venus, and Mercury do when viewed from Earth. As seen from Mars by MGS on 8 May 2003 at 13:00 GMT (6:00 AM PDT), Earth and the Moon appeared in the evening sky. The MOC Earth/Moon image has been specially processed to allow both Earth (with an apparent magnitude of -2.5) and the much darker Moon (with an apparent magnitude of +0.9) to be visible together. The bright area at the top of the image of Earth is cloud cover over central and eastern North America. Below that, a darker area includes Central America and the Gulf of Mexico. The bright feature near the center-right of the crescent Earth consists of clouds over northern South America. The image also shows the Earth-facing hemisphere of the Moon, since the Moon was on the far side of Earth as viewed from Mars. The slightly lighter tone of the lower portion of the image of the Moon results from the large and conspicuous ray system associated with the crater Tycho.

Credit:: NASA/JPL/Malin Space Science Systems

"Happy Face" Crater on Mars ¤õ¬P¡u¯ºÁy¡vÀô§Î¤s (23/5/2003)
¤õ¬P¤Wªº¤@­Ó©_©ÇÀô§Î¤s--¯ºÁyÀô§Î¤s¡C¥¿±`ªºÀô§Î¤s³£¬O¶ê§Îªº¡A¤¤¥¡©Î³\·|¬ð°_¡A¹³¥¦©P³ò¨º´X­Ó«K¬O¥¿±`ªº¡A¦ý³o­ÓÀô§Î¤s¼Ë¤l¯u¥i·R¡A¬O¤@­Ó¯ºÁy¡A¦³²´¦³¤f¡A´N¹³¬O¦Û¤vµe¤W¥hªº¡C³oÀô§Î¤s¡A¥¿¦W¬°GalleÀô§Î¤s¡A¥H¬ö©À¼w°ê¤Ñ¤å¾Ç®aJohann Galle¡Aª½®|230¤½¨½¡A¦ì©ó¤õ¬Pªº«n¥b²y¡CÀô§Î¤s¬O¹k¥Û¼²À»®É§Î¦¨ªº¡A¦a²y¤]¦³«Ü¦hÀô§Î¤s¡A¤ë²yªí­±«h§ó¦h¡C

Caption:: The picture show Galle Crater, informally known as "Happy Face," as it appeared in early southern winter. The white-ish gray surfaces are coated with wintertime carbon dioxide frost. The pattern of frost distribution gives the appearance that "Happy Face" has opened its mouth. Galle Crater is located on the east rim of Argyre at 51¢XS, 31¢XW. Sunlight illuminates the scene from the upper left. Galle Crater is 230 km (143 mi) across.

Credit:: NASA/JPL/Malin Space Science Systems

Eagle Nebula ÆNª¬¬P¶³ (22/5/2003)
¤£¸g¤£Ä±¤w¸g¸g¹L¤F8¦~¡A°O±o8¦~«e²Ä¤@¦¸¨£³o±i¬Û®É¥Ø©w¤f§b¡A½T¹ê¡A«Üè°¡C°£¤F¦â±mÄ}¯É¥~¡A¬P¶³¥»¨­ªº§ÎºA¤]«Ü¯S§O¡C¤§©Ò¥H¥s§@ÆNª¬¬P¶³¡A·íµM¬O¦]¬°¥¦¦ü¤@°¦ÆN¡A¤£¦ü¶Ü¡H¨ä¹ê¤S¯u¬O¤£©ö¬Ý¨ì¡A¦]¬°§A²{¦b¥u¬Ý¨ì¬P¶³ªº¤@³¡¥÷¡A¤S¬Oµ¥¦³¾÷·|§ä¥t¤@±iÆNª¬¬P¶³ªº¬Û¤W¨Ó¡]¤w³\¤U¤F¤£¤ÖªÅÀY¤ä²¼¤F¡A¦½¡^¡C³o¬P¶³¤S¦WM16¡]¬O¤@­Ó¬Pªíùتº½s¸¹¡^¡A¤]¬O¤@³B«í¬P½Ï¥Í¦a¡A¬P¶³¤¤ªº®ðÅé»P¹Ð®J¤@ª½¥¥¨|µÛªì¥Í«í¬P¡C°O±o¤£¥u¤@­Ó¤H°Ý¹L¡A·F¶Ü¹Ïªº¥k¤W¨¤·|¤F¤£¨£¤F¡A³o¬O¦]¬°«¢«k¤ÓªÅ±æ»·Ãè¦P®É¥Î4­Ó¬Û¾÷©çÄá¡A¤À§O­t³d¥ª¤W¡B¥k¤W¡B¥ª¤U©M¥k¤U4­Ó¦ì¸m¡A¦ý²Ä4­Ó¬Û¾÷ªºµø³õ¤ñ¨ä¾l3­Ó²Ó¤p¦Ó­P¡A«Ü¦h¦­´Áªº«¢«k·Ó¤ù³£¬O³o¼Ëªº¡C

Caption:: Eerie, dramatic pictures from the Hubble telescope show newborn stars emerging from "eggs" ¡X not the barnyard variety ¡X but rather, dense, compact pockets of interstellar gas called evaporating gaseous globules (EGGs). Hubble found the "EGGs," appropriately enough, in the Eagle nebula, a nearby star-forming region 7,000 light-years from Earth in the constellation Serpens. These striking pictures resolve the EGGs at the tip of finger-like features protruding from monstrous columns of cold gas and dust in the Eagle Nebula (also called M16). The columns ¡X dubbed "elephant trunks" ¡X protrude from the wall of a vast cloud of molecular hydrogen, like stalagmites rising above the floor of a cavern. Inside the gaseous towers, which are light-years long, the interstellar gas is dense enough to collapse under its own weight, forming young stars that continue to grow as they accumulate more and more mass from their surroundings.

Credit:: Jeff Hester and Paul Scowen (Arizona State University), and NASA

Tadpole Galaxy ½Á°B¬P¨t (21/5/2003)
¬P¨t¶¡ªº¸I¼²­ì¨Ó¬O«Ü¦hªº¡A¬Æ¦Ü¬O¥Ñ©ó¬P¨t¤§¶¡ªº¸I¼²¦Ó¥O¬P¨tºt¤Æ¡C³o­Ó½Á°B¬P¨t¶ZÂ÷§Ú­Ì420,000,000¥ú¦~¡]«Ü»·§a¡A·Q¹³¨ì¶Ü¡H¡^¡A¤S¬O¤@­Ó¬P¨t¸I¼²ªº¬¡¥Í¥Í¨Ò¤l¡A§A¨£¨ì¨º¦ù¥X¨Óªøªøªº§À¡A´N¬O¼²À»¡]¨ä¹ê¥¼¥²¤@©w¬O¥¿­±¼²¤W¡AÀ¿¹L¤]»¡¤£©w¡^®É³Q¹ï¤è±j¤jªº­«¤O§l¤Þ©Ô§è¥X¨Óªº¡A³o±ø§À¨¬¨¬¦³280,000¥ú¦~¡C°£¤F½Á°B¬P¨t¥~¡A§AÁÙ¥i¥H¨£¨ì«Ü¦h¤@ÂIÂI¡A¨ä¹ê¨CÂI§A¨£¨ìªº³£¬O¤@­Ó¬P¨t¡A¥u¬O¦]¬°¥¦­Ì¤ñ½Á°B§ó»·¡A¬Ý°_¨Ó§ó²Ó¦Ó¤w¡A³o¹Ï¤j¬ù¦³6000­Ó³o¼Ëªº­I´º¬P¨t¡C

Caption:: In this stunning vista recorded with the Hubble Space Telescope's new advanced camera, distant galaxies form a dramatic backdrop for disrupted spiral galaxy Arp 188, the Tadpole Galaxy. The cosmic Tadpole is a mere 420 million light-years distant toward the northern constellation Draco. Its eye-catching tail is about 280 thousand light-years long and features massive, bright blue star clusters. One story goes that a more compact intruder galaxy crossed in front of Arp 188 - from left to right in this view - and was slung around behind the Tadpole by their gravitational attraction. During the close encounter, tidal forces drew out the spiral galaxy's stars, gas, and dust forming the spectacular tail. The intruder galaxy itself, estimated to lie about 300 thousand light-years behind the Tadpole, can be seen through foreground spiral arms at the upper left. Following its terrestrial namesake, the Tadpole Galaxy will likely lose its tail as it grows older, the tail's star clusters forming smaller satellites of the large spiral galaxy.

Credit:: NASA, H. Ford (JHU), G. Illingworth (USCS/LO), M.Clampin (STScI), G. Hartig (STScI), the ACS Science Team, and ESA

Star Formation Region IC4678 «í¬P½Ï¥Í¦a IC4678 (20/5/2003)
°O±o³o±i¬Û´¿¸g°µ¹LScience´Á¥Zªº«Ê­±¡A¦Ó¸Ó´Á¥¿¥H«í¬P½Ï¥Í¬°±MÃD¡C¨ä¹ê«í¬P¸ò¤H¤@¼Ë¡A¦³¥Í¦Ñ¦ºªº¶¥¬q¡A¤µ¦¸´NÅý§Ú¨Ó¤¶²Ð¤@¨Ç½Ï¥Íªº¶¥¬q¡C«í¬Pªº¥ÀÅé´N¬O¬P»Ú¶³¡A¤@¨Ç§t¦³¤j¶q®ðÅé©M¹Ð®Jªº¦a¤è¡A·í¨º¨Ç¹Ð¶V»E¶V¦h®É¡A´N·|Åܬ°¬P¤F¡]«Ü¯«©_§a¡H¬Oªº¡A¦t©z¤¤«Ü¦hªF¦è³£³£«Ü¯«©_¡A¨ä¹ê¤¤¶¡ÁÙ¦³«Ü¥J²Óªº¹Lµ{¡A¯d«Ý¤é«á¦A¤¶²Ð§a¡^¡CIC4678¦ì©ó¤H°¨®y¤è¦V¡A¬P»Ú¶³±K«×°ª¡A¬O¤@­Ó«í¬P½Ï¥Í¦a¡A¬Û«H©ó¼Æ¦Ê¸U¦~«á¡A´N·|¦³«Ü¦h«í¬P½Ï¥Í¡C¡]¼Æ¦Ê¸U¦~¹ï©ó«í¬P¨Ó»¡¡A¬O«Üµu¼Èªº¡^

Caption:: This extremely rich region of our galaxy, IC 4678 area in the Sagittarius, illustrates brillantly the complex evolution cycle of matter in galaxies. Molecular clouds, seen here as the obscuring nebulae, eventually condense and turn into star formation regions. After millions of years, the new born stars will have blown their initial envelope back into the interstellar medium. Eventually, the cluster itself will dissolve, each star taking its own path into the galaxy's giant whirl, mixing with the previous generations of stars.

Credit:: Jean-Charles Cuillandre (CFHT) and CFHT


<<Next :: :: Home :: About :: Archive :: Index :: Guestbook :: Previous>>
 

PAGE :: 1    SITE :: 1    stardust.net :: 1

cheungszeleung@gmail.com LAST UPDATE: 25/5/2003