• → European Space Agency

      • Space for Europe
      • Space News
      • Space in Images
      • Space in Videos
    • About Us

      • Welcome to ESA
      • DG's News and Views
      • For Member State Delegations
      • Business with ESA
      • ESA Exhibitions
      • ESA Publications
      • Careers at ESA
    • Our Activities

      • Space News
      • Observing the Earth
      • Human Spaceflight
      • Launchers
      • Navigation
      • Space Science
      • Space Engineering
      • Operations
      • Technology
      • Telecommunications & Integrated Applications
    • For Public

    • For Media

    • For Educators

    • For Kids

    • ESA

    • Space in Images

    ESA > Space in Images > 2001 > 12 > Optical counterpart of the gamma-ray burst detected by Ulysses, Mars Odyssey and BeppoSAX

    Free Search (10906 images)

    • Recently Added
    • Advanced Search

    Optical counterpart of the gamma-ray burst detected by Ulysses, Mars Odyssey and BeppoSAX

    gamma-ray burst detected by Ulysses, Mars Odyssey and BeppoSAX
    Views: 1
    Rating: 0.00/5 (0 votes cast)

    Rate this Image

    • Currently 0 out of 5 Stars.
    • 1
    • 2
    • 3
    • 4
    • 5

    Thank you for rating!

    You have already rated this page, you can only rate it once!

    Your rating has been changed, thanks for rating!

    Share this Image

    Post to Facebook Post to MySpace Post to Delicious Post to Digg Post to Twitter

    Details

    Open/Close
    • Title Optical counterpart of the gamma-ray burst detected by Ulysses, Mars Odyssey and BeppoSAX
    • Released 18/02/2002 6:59 pm
    • Copyright M.Brown,R.Schommer,K.Olsen, B.Jannuzi,A.Dey(NOAO),A.Fruchter,J.Rhoads(STSci) AURA/NSF
    • Description

      The blue dot in the centre of this image (shown by the arrow) is the optical light signature of GRB011121, the gamma-ray burst detected by Ulysses, Mars Odyssey and BeppoSAX on 21 November 2001. The gamma-ray burst briefly appeared brighter than the rest of the Universe in gamma rays, before rapidly fading away.


      This optical image, taken with the National Science Foundation's Blanco 4-meter telescope at Cerro Tololo Inter-American Observatory in Chile during the morning of 23 November 2001, shows the optical transient a day and a half after the initial burst. The transient had faded in brightness from its peak by more than a factor of 100 in that period of time. The reddish dot adjoining the gamma-ray burst, at its lower left, is probably the core of the galaxy in which the gamma-ray burst occurred.


      photo: M.Brown,R.Schommer,K.Olsen, B.Jannuzi,A.Dey(NOAO),A.Fruchter,J.Rhoads(STSci) AURA/NSF


    TAGS

    Open/Close
    • Click on the tags to find the matching images.
    • Activity Space Science
    • Mission Ulysses
    • Keywords Astronomy techniques

    TAGS

    Open/Close

    Details

    Open/Close

    RELATED IMAGES

    • Gamma-ray bursts
      A gamma-ray burst
      Released: 15/02/2006
      Rating
    • Gamma-ray bursts
      Gamma-ray bursts
      Released: 15/02/2006
      Rating

    Connect with us

    • RSS
    • Youtube
    • Twitter
    • Flickr
    • Google Buzz
    • Facebook
    • Livestream
    • Subscribe
    • App Store
    • LATEST ARTICLES
    • · ESA astronaut Timothy Peake set …
    • · Space drives e-mobility
    • · Proba-V opens its eyes
    • · First new Galileo satellite arri…
    • · Next destination: space
    • FAQ

    • Jobs at ESA

    • Site Map

    • Contacts

    • Terms and conditions