NASA 03月12日
NGC 772: The Fiddlehead Galaxy
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这张天文每日一图展示了NGC 772,也被称为卷须星系,它奇特的螺旋形状源于与附近椭圆星系NGC 770的引力互动。虽然卷须星系距离我们1亿光年,跨度超过20万光年,但图中还出现了一颗“不速之客”——彗星43P/Wolf-Harrington。这颗彗星实际上离我们更近,仅几光分之遥,位于太阳系内。虽然从视角上看,彗星似乎正朝着星系飞去,但它们之间并没有物理联系,这只是一个难得的巧合,让这两个宇宙奇观在法国卡莱恩的夜空中同框。

🌌NGC 772,又名卷须星系,其独特的卷曲外形归因于与邻近椭圆星系NGC 770的引力相互作用,它们之间的引力“舞蹈”塑造了星系的形态。

🔭卷须星系距离地球约1亿光年,横跨超过20万光年,在天空中的位置位于白羊座。它被编录为NGC 772和Arp 78。

☄️彗星43P/Wolf-Harrington看似正对着遥远的星系,实则不然。它位于太阳系内,距离我们仅几光分,与星系之间并无实际关联,只是观测视角上的重合。

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2025 March 12

NGC 772: The Fiddlehead Galaxy
Image Credit & Copyright: Jean-François Bax & Serge Brunier, OCA/C2PU; Text: Ogetay Kayali (Michigan Tech U.)

Explanation: Why does this galaxy look like a curly vegetable? The Fiddlehead spiral galaxy likely gets its distorted spiral appearance from a gravitational interaction with its close-by elliptical companion NGC 770, seen just below. Cataloged as NGC 772 and Arp 78, the Fiddlehead spans over 200,000 light years, is a nearby 100 million light years beyond the stars of our Milky Way galaxy, and is visible toward the constellation of the Ram (Aries). But in the featured image, the Fiddlehead appears to have another companion -- one with a long and fuzzy tail: Comet 43P/Wolf-Harrington. Though the comet appears to be aimed straight at the massive galaxy, it is actually much closer to us, residing only light minutes away -- well within our Solar System. The comet will never reach the distant spiral galaxy, nor is it physically related to it. By a fortunate trick of perspective, though, these two cosmic wonders briefly share the same frame taken late last year from Calern, France.

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NGC 772 卷须星系 彗星43P/Wolf-Harrington
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