File:A Young Pulsar Shows its Hand.jpg

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Description: At the center of this Chandra image, a pulsar -- only twelve miles in diameter -- is responsible for this X-ray nebula that spans 150 light years. This pulsar is spinning around almost 7 times a second and has a magnetic field at its surface estimated to be 15 trillion times stronger than the Earth's magnetic field. This combination of rapid rotation and ultra-strong magnetic field drives an energetic wind of electrons and ions, ultimately creating the elaborate nebula seen by Chandra.

Creator/Photographer: Chandra X-ray Observatory

NASA's Chandra X-ray Observatory, which was launched and deployed by Space Shuttle Columbia on July 23, 1999, is the most sophisticated X-ray observatory built to date. The mirrors on Chandra are the largest, most precisely shaped and aligned, and smoothest mirrors ever constructed. Chandra is helping scientists better understand the hot, turbulent regions of space and answer fundamental questions about origin, evolution, and destiny of the Universe. The images Chandra makes are twenty-five times sharper than the best previous X-ray telescope. NASA's Marshall Space Flight Center in Huntsville, Ala., manages the Chandra program for NASA's Science Mission Directorate in Washington. The Smithsonian Astrophysical Observatory controls Chandra science and flight operations from the Chandra X-ray Center in Cambridge, Massachusetts.

Medium: Chandra telescope x-ray

Date: 2009

Persistent URL: [1]

Repository: Smithsonian Astrophysical Observatory

Gift line: NASA/CXC/SAO/P.Slane, et al.

Accession number: PSR B1509-58
日期
來源 A Young Pulsar Shows its Hand
作者 Smithsonian Institution from United States
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這幅圖片原始出處為Flickr的https://www.flickr.com/photos/25053835@N03/3424495044 ,作者為Smithsonian Institution 。經機器人FlickreviewR在2009年7月28日審查後確定為採用No known copyright restrictions的協議授權使用。

2009年7月28日

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目前2009年7月28日 (二) 03:36於 2009年7月28日 (二) 03:36 版本的縮圖1,200 × 1,200(562 KB)Raeky{{Information |Description= '''Description''': At the center of this Chandra image, a pulsar -- only twelve miles in diameter -- is responsible for this X-ray nebula that spans 150 light years. This pulsar is spinning around almost 7 times a second and ha

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