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 language | English |
|---|---|
| Pages (from-to) | 16-24 |
| Number of pages | 9 |
| Journal | The Messenger |
| Issue number | 143 |
| Publication status | Published - Mar 2011 |
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