Resumo (PT):
Abstract (EN):
GRAVITY is the second generation Very
Large Telescope Interferometer instrument for precision narrow-angle as -
trometry 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.
Language:
English
Type (Professor's evaluation):
Scientific
No. of pages:
9