The High Accuracy Radial Velocity Planet Searcher (HARPS) is a high-precision
echelle planet-finding
spectrograph
An optical spectrometer (spectrophotometer, spectrograph or spectroscope) is an instrument used to measure properties of light over a specific portion of the electromagnetic spectrum, typically used in spectroscopic analysis to identify mate ...
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
exoplanet
An exoplanet or extrasolar planet is a planet outside the Solar System. The first possible evidence of an exoplanet was noted in 1917 but was not recognized as such. The first confirmation of detection occurred in 1992. A different planet, init ...
s to date, with the first one in 2004, making it the most successful planet finder behind the
Kepler space observatory. It is a second-generation
radial-velocity spectrograph, based on experience with the
ELODIE and
CORALIE
Coralie is a French feminine name meaning "coral", derived from the Latin word ''coralium''.Also spelt ''corallum'', ''corallium'' or ''curalium'', cf.br>Whitaker's Words/ref> It was the eighth most popular name for baby girls in Quebec in 2007.
N ...
instruments.
Characteristics
The HARPS can attain a precision of 0.97 m/s (3.5 km/h),
making it one of only two instruments worldwide with such accuracy. 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. The precision and sensitivity of the instrument is such that it incidentally produced the best available measurement of the thorium spectrum. Planet-detection is in some cases limited by the
seismic pulsations of the star observed rather than by limitations of the instrument.
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.
It was initially used for a survey of one-thousand stars.
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.
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.
;Notes:
* (a) — M ''sin i''
brown dwarf
* (b) — brown dwarf
* (c) — shorter period
Gallery
File:The HELIOS instrument at the ESO 3.6-metre telescope in Chile.jpg, HELIOS instrument installed to feed sunlight via fibre optics to the HARPS
File:A decade of discoveries from HARPS.jpg, A decade of discoveries from HARPSHD 10180
HD 10180, also designated 2MASS J01375356-6030414, is a Sun-like star in the southern constellation Hydrus that is notable for its large planetary system. Since its discovery, at least six exoplanets have been observed orbiting it, and ...
with its seven planets
See also
Similar instruments:
*
HARPS-N is a copy of this instrument installed in the northern hemisphere in 2012.
*
HARPS3 is an updated design of this instrument that will be installed on an upgraded and roboticised Isaac Newton Telescope, in 2024.
*
Fiber-optic Improved Next-generation Doppler Search for Exo-Earths, operating at Lick observatory since 2009
*
Anglo-Australian Planet Search or ''AAPS'' is another southern hemisphere planet search program.
*
ESPRESSO is a new-generation spectrograph for
ESO's
VLT.
*
Automated Planet Finder, at the Lick observatory, commissioned in 2013.
*CAFE (Calar Alto Fibre-fed Echelle spectrograph) installed on the Calar Alto Observatory's 2.2-metre telescope in 2014, and the
CARMENES
The CARMENES survey (Calar Alto high-Resolution search for M-dwarfs with Exoearths with Near-infrared and optical Échelle Spectrographs) is a project to examine approximately 300 M-dwarf stars for signs of exoplanets with the CARMENES instrument o ...
mounted on the 3.5-metre telescope in 2016.
*
EXPRES The EXtreme PREcision Spectrograph (EXPRES) is an optical fiber fed echelle instrument designed and built at the Yale Exoplanet Laboratory to be installed on the 4.3-meter Lowell Discovery Telescope operated by Lowell Observatory. It has a goal t ...
is a third generation radial velocity spectrograph that is planned to be installed on the
Lowell Discovery Telescope.
Space based detectors :
*
COROT, spacecraft operating since 2007
*
Kepler, operational since 2009
*
Terrestrial Planet Finder, not funded, probably cancelled
*
Space Interferometry Mission
The Space Interferometry Mission, or SIM, also known as SIM Lite (formerly known as SIM PlanetQuest), was a planned space telescope proposed by the U.S. National Aeronautics and Space Administration (NASA), in conjunction with contractor Northro ...
, construction halted in 2010
*
Darwin
Darwin may refer to:
Common meanings
* Charles Darwin (1809–1882), English naturalist and writer, best known as the originator of the theory of biological evolution by natural selection
* Darwin, Northern Territory, a territorial capital city i ...
, early studies for a multi-satellite mission
References
External links
*
*
* ''(Contains list of discoveries from 2005 survey.)''
*
*
{{Exoplanet search projects
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