File:Messier22.jpg
Original file (2,400 × 3,000 pixels, file size: 495 KB, MIME type: image/jpeg)
Captions
Globular cluster Messier 22
Summary
[edit]From NASA Press Release June 27, 2001 02:00 PM (EDT) News Release Number: STScI-2001-20 Hint of Planet-Sized Drifters Bewilders Hubble Scientists
- Piercing the heart of a glittering swarm of stars, NASA's sharp-eyed Hubble Space Telescope unveils the central region of the globular cluster M22, a 12- to 14-billion-year-old grouping of stars in the constellation Sagittarius. The telescope's view of the cluster's core measures 3.3 light-years across.
- The stars near the cluster's core are 100,000 times more numerous than those in the Sun's neighborhood. Buried in the glow of starlight are about six "mystery objects," which astronomers estimate are no larger than one quarter the mass of the giant planet Jupiter, the solar system's heftiest planet.
- The mystery objects are too far and dim for Hubble to see directly. Instead, the orbiting observatory detected these unseen celestial bodies by looking for their gravitational effects on the light from far distant stars. In this case, the stars are far beyond the cluster in the galactic bulge, about 30,000 light-years from Earth at the center of the Milky Way Galaxy. M22 is 8,500 light-years away. The invisible objects betrayed their presence by bending the starlight gravitationally and amplifying it, a phenomenon known as microlensing.
- From February 22 to June 15, 1999, Hubble's Wide Field and Planetary Camera 2 looked through this central region and monitored 83,000 stars. During that time the orbiting observatory recorded six unexpectedly brief microlensing events. In each case a background star jumped in brightness for less than 20 hours before dropping back to normal. These transitory spikes in brightness mean that the object passing in front of the star must have been much smaller than a normal star. Hubble also detected one clear microlensing event. In that observation a star appeared about 10 times brighter over an 18-day span before returning to normal. Astronomers traced the leap in brightness to a dwarf star in the cluster floating in front of the background star.
- The inset photo shows the entire globular cluster of about 10 million stars. M22 is about 60 light-years wide. The image was taken in June 1995 by the Burrell Schmidt telescope at the Case Western Reserve University's Warner and Swasey Observatory on Kitt Peak in Arizona.
- Object Name: M22
- Image Type: Astronomical
- Credits for the Hubble image: NASA, Kailash Sahu, Stefano Casertano, Mario Livio, Ron Gilliland (Space Telescope Science Institute), Nino Panagia (European Space Agency/Space Telescope Science Institute), Michael Albrow and Mike Potter (Space Telescope Science Institute)
- Credits for ground-based image: Nigel A.Sharp, REU program/AURA/NOAO/NSF
Licensing
[edit]Public domainPublic domainfalsefalse |
This file is in the public domain in the United States because it was solely created by NASA. NASA copyright policy states that "NASA material is not protected by copyright unless noted". (See Template:PD-USGov, NASA copyright policy page or JPL Image Use Policy.) | ||
Warnings:
|
File history
Click on a date/time to view the file as it appeared at that time.
Date/Time | Thumbnail | Dimensions | User | Comment | |
---|---|---|---|---|---|
current | 22:07, 7 November 2006 | 2,400 × 3,000 (495 KB) | WilliamKF (talk | contribs) | http://hubblesite.org/newscenter/archive/releases/2001/20/image/a {{PD-USGov-NASA}} | |
15:35, 1 February 2005 | 165 × 165 (8 KB) | CWitte (talk | contribs) | Messier 22 |
You cannot overwrite this file.
File usage on Commons
The following 2 pages use this file:
File usage on other wikis
The following other wikis use this file:
- Usage on af.wikipedia.org
- Usage on be.wikipedia.org
- Usage on bg.wikipedia.org
- Usage on co.wikipedia.org
- Usage on el.wikipedia.org
- Usage on en.wikipedia.org
- Usage on en.wikibooks.org
- Usage on fr.wikipedia.org
- Usage on id.wikipedia.org
- Usage on it.wikipedia.org
- Usage on ko.wikipedia.org
- Usage on lb.wikipedia.org
- Usage on li.wikipedia.org
- Usage on lt.wikipedia.org
- Usage on nl.wikipedia.org
- Usage on pt.wikipedia.org
- Usage on ro.wikipedia.org
- Usage on ru.wikipedia.org
- Usage on sh.wikipedia.org
- Usage on sk.wikipedia.org
- Usage on sr.wikipedia.org
- Usage on vi.wikipedia.org
Metadata
This file contains additional information such as Exif metadata which may have been added by the digital camera, scanner, or software program used to create or digitize it. If the file has been modified from its original state, some details such as the timestamp may not fully reflect those of the original file. The timestamp is only as accurate as the clock in the camera, and it may be completely wrong.
_error | 0 |
---|