原始文件 (3,921 × 3,921像素,文件大小:23.03 MB,MIME类型:image/jpeg


描述
English: Astronomers using NASA's Hubble Space Telescope have discovered a ghostly ring of dark matter that formed long ago during a titanic collision between two massive galaxy clusters. The ring's discovery is among the strongest evidence yet that dark matter exists. Astronomers have long suspected the existence of the invisible substance as the source of additional gravity that holds together galaxy clusters. Such clusters would fly apart if they relied only on the gravity from their visible stars. Although astronomers don't know what dark matter is made of, they hypothesize that it is a type of elementary particle that pervades the universe.
This Hubble composite image shows the ring of dark matter in the galaxy cluster CL 0024+17. The ring-like structure is evident in the blue map of the cluster's dark matter distribution. The map was derived from Hubble observations of how the gravity of the cluster Cl 0024+17 distorts the light of more distant galaxies, an optical illusion called gravitational lensing. Although astronomers cannot see dark matter, they can infer its existence by mapping the distorted shapes of the background galaxies. The map is superimposed on a Hubble Advanced Camera for Surveys image of the cluster taken in November 2004.
Slovenščina: Prstenec tmavej hmoty v kope galaxií CL0024+17. Snímku zhotovil Hubblov vesmírny ďalekohľad v novembri 2004. Prstenec tmavej hmoty má priemer 5 miliónov svetelných rokov. Vznikol pravdepodobne zrážkou dvoch kôp galaxií. (kľúčové slová: tmavá hmota, galaxia, alebo CL0024+17, dark matter, gravitational lensing).
日期
来源 http://hubblesite.org/newscenter/archive/releases/2007/17/image/a/ (direct link)
作者 NASA, ESA, M.J. Jee and H. Ford (Johns Hopkins University)
授权
(二次使用本文件)
Public domain
This file is in the public domain because it was created by NASA and ESA. NASA Hubble material (and ESA Hubble material prior to 2009) is copyright-free and may be freely used as in the public domain without fee, on the condition that only NASA, STScI, and/or ESA is credited as the source of the material. This license does not apply if ESA material created after 2008 or source material from other organizations is in use.

The material was created for NASA by Space Telescope Science Institute under Contract NAS5-26555, or for ESA by the Hubble European Space Agency Information Centre. Copyright statement at hubblesite.org or 2008 copyright statement at spacetelescope.org.

For material created by the European Space Agency on the spacetelescope.org site since 2009, use the {{ESA-Hubble}} tag.
其他版本
Original Hubble image

Side-by-side original and enhanced HUBBLE dark matter halo
注解
InfoField
该图片含有注解:在维基媒体共享资源上查看注解

说明

添加一行文字以描述该文件所表现的内容

此文件中描述的项目

描绘内容

媒体类型 简体中文(已转写)

image/jpeg

校验和 简体中文(已转写)

005ca77447892b2f6cc3b8e08432e380398ac140

断定方法:​SHA-1 简体中文(已转写)

数据大小 简体中文(已转写)

24,147,234 字节

3,921 像素

3,921 像素

文件历史

点击某个日期/时间查看对应时刻的文件。

日期/时间缩⁠略⁠图大小用户备注
当前2009年7月19日 (日) 13:332009年7月19日 (日) 13:33版本的缩略图3,921 × 3,921(23.03 MB)TryphonOriginal size.
2007年5月17日 (四) 01:362007年5月17日 (四) 01:36版本的缩略图1,280 × 1,280(1.75 MB)Clh288~commonswiki{{Information |Description=Astronomers using NASA's Hubble Space Telescope have discovered a ghostly ring of dark matter that formed long ago during a titanic collision between two massive galaxy clusters. The ring's discovery is among the strongest evide

全域文件用途

元数据