High Accuracy Radial Velocity Planet Searcher

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File:HARPS Spectrograph and the 3.6m Telescope.jpg
Montage of the HARPS spectrograph and the 3.6m telescope at La Silla. The upper left shows the dome of the telescope, while the upper right illustrates the telescope itself. The HARPS spectrograph is shown in the lower image during laboratory tests. The vacuum tank is open so that some of the high-precision components inside can be seen

The High Accuracy Radial Velocity Planet Searcher (HARPS) is a high-precision echelle planet-finding spectrograph installed in 2002 on the ESO's 3.6m telescope at La Silla Observatory in Chile. The first light was achieved in February 2003. HARPS has discovered over 130 exoplanets to date, with the first one in 2004, making it the most successful planet finder behind the Kepler space telescope. It is a second-generation radial-velocity spectrograph, based on experience with the ELODIE and CORALIE instruments.[1]

Characteristics

The HARPS can attain a precision of 0.97 m/s (3.5 km/h),[2] making it one of only two instruments worldwide with such accuracy.Script error: No such module "Unsubst". This is due to a design in which the target star and a reference spectrum from a thorium lamp are observed simultaneously using two identical optic fibre feeds, and to careful attention to mechanical stability: the instrument sits in a vacuum vessel which is temperature-controlled to within 0.01 kelvins.[3] The precision and sensitivity of the instrument is such that it incidentally produced the best available measurement of the thorium spectrum.Script error: No such module "Unsubst". Planet-detection is in some cases limited by the seismic pulsations of the star observed rather than by limitations of the instrument.[4]

The principal investigator on the HARPS is Michel Mayor who, along with Didier Queloz and Stéphane Udry, have used the instrument to characterize the Gliese 581 planetary system, home to one of the smallest known exoplanets orbiting a normal star, and two super-Earths whose orbits lie in the star's habitable zone.[5]

It was initially used for a survey of one-thousand stars.Script error: No such module "Unsubst".

Since October 2012 the HARPS spectrograph has the precision to detect a new category of planets: habitable super-Earths. This sensitivity was expected from simulations of stellar intrinsic signals, and actual observations of planetary systems. Currently, the HARPS can detect habitable super-Earth only around low-mass stars as these are more affected by gravitational tug from planets and have habitable zones close to the host star.[6]

Discoveries

This is an incomplete list of exoplanets discovered by the HARPS. The list is sorted by the date of the discovery's announcement. As of December 2017, the list contains 134 exoplanets.

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Gallery

See also

File:Sparkling Ribbon of Stars — The Southern Milky Way over La Silla.jpg
ESO 3.6-metre telescope is home to the world's foremost exoplanet hunter, HARPS.[9]

Similar instruments:

Space based detectors :

Notes

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References

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External links

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