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標題: 宇宙級的龍捲風 [打印本頁]

作者: starsue1211    時間: 2010-8-25 00:35     標題: 宇宙級的龍捲風

      Light-years in length, this cosmic tornado is actually a powerful jet cataloged as HH (Herbig-Haro) 49/50 blasting down from the top of a Spitzer Space Telescope view. Though such energetic outflows are well known to be associated with the formation of young stars, the exact cause of the spiraling structures apparent in this case is still mysterious. The embryonic star responsible for the 100-kilometer per second jet is located just off the top of the picture, while the bright star seen near the tip of the jet may just by chance lie along the line of sight. In the false-color infrared image, the tornado glows with infrared light generated as the outflow heats surrounding dust clouds. The color coding shows a trend from red to blue hues at the tornado's tip indicating a systematic increase in emission at shorter wavelengths. The trend is thought to indicate an increase in molecular excitation closer to where the head of the jet is impacting interstellar gas. HH49/50 is about 450 light-years distant, located in the Chamaeleon I molecular cloud.  

      這道長數光年的宇宙級龍捲風,實際上是一道編號為HH49/50的強大噴流,它從這幅史匹哲太空望遠鏡影像的上端向下噴。雖然這種強大的物質噴流通常和年輕恆星的形成過程有關,但像這個範例中的螺旋結構到底是怎麼造成的,則仍然未知。造成這道秒速一百公里噴流的胎星,位在這幅影像頂端的外頭,而噴流頂點附近的亮星可能只是湊巧位在同一個方向而已。在這張假色紅外光影像裡,噴流之所會發出紅外輻射,是來自被噴流所加熱的周遭塵埃雲氣。這道噴流頂點的色澤由紅漸次轉變成藍色,顯示所發出的短波長輻射系統性地循序增強。一般認為這種取向顯示愈靠近噴流頂點,噴流衝撞星際雲所所造成的分子激發也愈強烈。HH49/50位在堰蜓座 (Chamaeleon)一號分子雲內,距離我們約有450光年遠。(HH = Herbig-Haro -- 赫比格-赫羅)

資料來源: Scientific American
               Department of Physics, NCKU


[ 本帖最後由 starsue1211 於 2010-8-25 00:36 編輯 ]

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