SPHERE

E176895

SPHERE is a high-contrast imaging instrument on the Very Large Telescope designed primarily for directly observing and characterizing exoplanets and circumstellar disks.

All labels observed (1)

Label Occurrences
SPHERE canonical 2

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Statements (47)

Predicate Object
instanceOf astronomical instrument
exoplanet imaging instrument
high-contrast imaging instrument
achievesContrast up to about 10^-6 at small angular separations
acronymFor Spectro-Polarimetric High-contrast Exoplanet REsearch
commissionedOn 2014
designedFor high-contrast imaging close to bright stars
fieldOfView small field optimized for nearby stars
firstLight 2014
fullName Spectro-Polarimetric High-contrast Exoplanet REsearch
fundedBy European Southern Observatory member states
hasSubsystem IFS
IRDIS
SAXO
ZIMPOL
installedOn Very Large Telescope
surface form: VLT UT3 Nasmyth platform
locatedAt Paranal Observatory
locatedIn Atacama Desert
Chile
observesWavelengthRange near-infrared
visible
operatedAt Very Large Telescope
operatedBy European Southern Observatory
partOf Very Large Telescope
surface form: Very Large Telescope instrumentation suite
primaryPurpose characterization of exoplanets
direct imaging of exoplanets
scienceGoal detection of faint companions near bright stars
study of circumstellar dust disks
study of exoplanet atmospheres
study of planet formation
secondaryPurpose imaging of circumstellar disks
subsystemFullName IFS – Integral Field Spectrograph
IRDIS – Infra-Red Dual-beam Imager and Spectrograph
SAXO – SPHERE AO for eXoplanet Observation
ZIMPOL – Zurich IMaging POLarimeter
supportsMode imaging
low-resolution spectroscopy
polarimetry
targetType nearby young stars
stars with debris disks
stars with protoplanetary disks
telescopeUnit Very Large Telescope
surface form: VLT Unit Telescope 3
telescopeUnitName Melipal
usesTechnique coronagraphy
differential imaging
extreme adaptive optics
polarimetric imaging

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Referenced by (2)

Full triples — surface form annotated when it differs from this entity's canonical label.