Magnification with a Gravitational Lens?引力透镜的放大效应?
One of the most distant observed objects in the universe, 13.4 billion light years, was observed with the help of the gravitational lens effect. The experimenters report an effective magnification of about 30, which allowed them to observe an object which would otherwise have been undetectable. 宇宙中观测到的最遥远的天体之一距离地球134亿光年,借助引力透镜效应进行了观测。实验人员报告了约30倍的有效放大率,使他们能够观测到原本无法检测到的天体。
![]() This NASA/ESA Hubble Space Telescope image shows a newly discovered very small, faint galaxy 'building block' found via a unique collaboration between ground- and space-based telescopes. Hubble and the 10 metre Keck Telescopes in Hawaii joined forces using a galaxy cluster which acts as a gravitational lens to detect what scientists believe is one of the smallest and most distant objects ever found. The galaxy cluster Abell 2218 was used by a team of European and American astronomers led by Richard Ellis (Caltech, USA) in their systematic search for intrinsically faint distant star-forming systems. Without the help from this cluster's magnifying power (it magnifies by around 30 times) the galaxy building block would have been undetectable with present facilities. In the image to the right, the object is seen distorted into two nearly identical, very red 'images' by the gravitational lens. The image pair represents the magnified result of a single background object gravitationally lensed by Abell 2218 and viewed at a distance of 13.4 billion light-years. The intriguing object contains only one million stars, far fewer than a mature galaxy, and Ellis and co-workers believe it is very young. Such young star-forming systems of low mass at early cosmic times are likely to be the objects from which the mature galaxies around us today have formed. In the image to the left, the full overview of the galaxy cluster Abell 2218 is seen. This image was taken by Hubble in 1999 during the Early Release Observations made immediately after the Hubble Servicing Mission 3A. Credit: ESA, NASA, Richard Ellis (Caltech, USA) and Jean-Paul Kneib (Observatoire Midi-Pyrenees, France)" 这张由NASA/ESA哈勃太空望远镜拍摄的图像显示了一个新发现的非常小而暗淡的星系‘构建块’,该发现是通过地面望远镜和空间望远镜之间的独特合作找到的。哈勃空间望远镜与夏威夷的10米凯克望远镜联合工作,利用一个星系团作为引力透镜,以探测科学家认为是迄今为止发现的最小且最遥远的天体之一。由理查德·埃利斯(美国加州理工学院)领导的欧洲和美国天文学家团队,利用阿贝尔2218星系团进行系统性搜索,寻找本质上暗淡的遥远恒星形成系统。如果没有这个星系团的放大作用(它放大了约30倍),这个星系构建块将无法被现有的设备检测到。在图像右侧,该天体被引力透镜扭曲成两个几乎相同且非常红的‘图像’。这对图像代表了由阿贝尔2218星系团引力透镜放大后的单一背景天体,其距离为134亿光年。这个引人注目的天体仅包含一百万颗恒星,远少于成熟星系,埃利斯和他的同事们认为它非常年轻。这种在宇宙早期低质量的年轻恒星形成系统,很可能是我们今天周围成熟星系的来源。在图像左侧,可以看到阿贝尔2218星系团的全景。这张图像由哈勃于1999年在早期释放观测期间拍摄,是在哈勃 servicing 任务3A之后立即进行的。版权:ESA,NASA,理查德·埃利斯(美国加州理工学院)和让-皮埃尔·涅比(法国 Midi-Pyrenees 观测站)
|
Index References 索引参考 | ||
|
Go Back
返回 |