원본 파일(2,400 × 3,000 픽셀, 파일 크기: 495 KB, MIME 종류: image/jpeg)

Globular cluster Messier 22

파일 설명

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

라이선스

Public domain 이 파일은 NASA에서 제작하였으므로 퍼블릭 도메인입니다. NASA의 저작권 정책에 따르면 NASA의 자료는 명시하지 않는 이상 저작권의 보호를 받지 않습니다. (Template:PD-USGov, 또는 NASA 저작권 정책 문서, JPL 그림 사용 정책을 참고하세요.)
주의사항:

파일 역사

날짜/시간 링크를 클릭하면 해당 시간의 파일을 볼 수 있습니다.

날짜/시간섬네일크기사용자설명
현재2006년 11월 8일 (수) 07:072006년 11월 8일 (수) 07:07 판의 섬네일2,400 × 3,000 (495 KB)WilliamKFhttp://hubblesite.org/newscenter/archive/releases/2001/20/image/a {{PD-USGov-NASA}}
2005년 2월 2일 (수) 00:352005년 2월 2일 (수) 00:35 판의 섬네일165 × 165 (8 KB)CWitteMessier 22

다음 문서 1개가 이 파일을 사용하고 있습니다:

이 파일을 사용하고 있는 모든 위키의 문서 목록

다음 위키에서 이 파일을 사용하고 있습니다:

메타데이터