GRAVITY: Observing the Universe in Motion

  • Frank Eisenhauer
  • , Guy Perrin
  • , Wolfgang Brandner
  • , Christian Straubmeier
  • , Karine Perraut
  • , Antonio Amorim
  • , Markus Schöller
  • , Stefan Gillessen
  • , Pierre Kervella
  • , Myriam Benisty
  • , Constanza Araujo-Hauck
  • , Laurent Jocou
  • , Jorge Lima
  • , Gerd Jakob
  • , Marcus Haug
  • , Yann Clénet
  • , Thomas Henning
  • , Andreas Eckart
  • , Jean Philippe Berger
  • , Paulo J. V. Garcia
  • Roberto N. Abuter, Stefan Kellner, Thibaut Paumard, Stefan Hippler, Sebastian Fischer, Thibaut Moulin, Jaime Villate, Gerardo Avila, Alexander Gräter, Sylvestre Lacour, Armin Huber, Michael Wiest, Axelle Nolot, Pedro Carvas, Reinhold Dorn, Oliver Pfuhl, Eric Gendron, Sarah Kendrew, Senol Yazici, Sonia Anton, Yves Jung, Markus Thiel, Élodie Choquet, Ralf Klein, Paula Stella Teixeira, Philippe Gitton, David Moch, Frederic Vincent, Natalia Kudryavtseva, Stefan Ströbele, Eckhard Sturm, Pierre Fédou, Rainer Lenzen, Paul Jolley, Clemens Kister, Vincent Lapeyrère, Vianak Naranjo, Christian Lucuix, Reiner Hofmann, Frederic Chapron, Udo Neumann, Leander Mehrgan, Oliver Hans, Gerard Rousset, Jose Ramos, Marcos Suarez, Reinhard Lederer, Jean Michel Reess, Ralf Rainer Rohloff, Pierre Haguenauer, Hendrik Bartko, Arnaud Sevin, Karl Wagner, Jean Louis Lizon, Sebastian Rabien, Claude Collin, Gert Finger, Richard Davies, Daniel Rouan, Markus Wittkowski, Katie Dodds-Eden, Denis Ziegler, Frederic Cassaing, Henri Bonnet, Mark Casali, Reinhardt Genzel, Pierre Lena

Research output: Contribution to journalArticle

Abstract

GRAVITY is the second generation Very Large Telescope Interferometer instrument for precision narrow-angle astrometry and interferometric imaging. With its fibre-fed integrated optics, wavefront sensors, fringe tracker, beam stabilisation and a novel metrology concept, GRAVITY will push the sensitivity and accuracy of astrometry and interferometric imaging far beyond what is offered today. Providing precision astrometry of order 10 microarcseconds, and imaging with 4-milliarcsecond resolution, GRAVITY will revolutionise dynamical measurements of celestial objects: it will probe physics close to the event horizon of the Galactic Centre black hole; unambiguously detect and measure the masses of black holes in massive star clusters throughout the Milky Way; uncover the details of mass accretion and jets in young stellar objects and active galactic nuclei; and probe the motion of binary stars, exoplanets and young stellar discs. The instrument capabilities of GRAVITY are outlined and the science opportunities that will open up are summarised.
Original languageEnglish
Pages (from-to)16-24
Number of pages9
JournalThe Messenger
Issue number143
Publication statusPublished - Mar 2011

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