The Haute-Provence Observatory (OHP, ) is an
astronomical observatory in the southeast of France, about 90 km east of
Avignon
Avignon (, , ; or , ; ) is the Prefectures in France, prefecture of the Vaucluse department in the Provence-Alpes-Côte d'Azur region of southeastern France. Located on the left bank of the river Rhône, the Communes of France, commune had a ...
and 100 km north of
Marseille
Marseille (; ; see #Name, below) is a city in southern France, the Prefectures in France, prefecture of the Departments of France, department of Bouches-du-Rhône and of the Provence-Alpes-Côte d'Azur Regions of France, region. Situated in the ...
. It was established in 1937 as a national facility for
French astronomer
An astronomer is a scientist in the field of astronomy who focuses on a specific question or field outside the scope of Earth. Astronomers observe astronomical objects, such as stars, planets, natural satellite, moons, comets and galaxy, galax ...
s. Astronomical observations began in 1943 using the 1.20 m
telescope
A telescope is a device used to observe distant objects by their emission, Absorption (electromagnetic radiation), absorption, or Reflection (physics), reflection of electromagnetic radiation. Originally, it was an optical instrument using len ...
, and the first research papers based on observations made at the observatory were published in 1944. Foreign observers first used the observatory in 1949, when
Geoffrey and
Margaret Burbidge visited.
The observatory lies at an altitude of about 650 m, on a
plateau
In geology and physical geography, a plateau (; ; : plateaus or plateaux), also called a high plain or a tableland, is an area of a highland consisting of flat terrain that is raised sharply above the surrounding area on at least one side. ...
near the village of
Saint-Michel-l'Observatoire in the
Alpes-de-Haute-Provence
Alpes-de-Haute-Provence (sometimes abbreviated as AHP; ; ; ), formerly until 1970 known as Basses-Alpes (, ), is a department in the Provence-Alpes-Côte d'Azur region of France, bordering Alpes-Maritimes and Italy to the east, Var to the sou ...
''
département''.
The site was chosen for an observatory because of its generally very favourable observing conditions. On average, 60% of nights are suitable for astronomical observations, with the best seasons being summer and autumn. About 170 nights per year on average are completely
cloud
In meteorology, a cloud is an aerosol consisting of a visible mass of miniature liquid droplets, frozen crystals, or other particles, suspended in the atmosphere of a planetary body or similar space. Water or various other chemicals may ...
less. The
seeing is usually around 2" but can reach 1" or lower on occasion. Seeing degrades severely, sometimes to over 10", when the cold
Mistral wind blows from the northwest. This happens on about 45 days per year on average, mostly during winter. Good weather conditions often follow a
Mistral. On average, atmospheric absorption at OHP is roughly twice that seen at the
European Southern Observatory
The European Organisation for Astronomical Research in the Southern Hemisphere, commonly referred to as the European Southern Observatory (ESO), is an intergovernmental organization, intergovernmental research organisation made up of 16 m ...
(ESO) at
La Silla, Chile.
The main-belt asteroid
7755 Haute-Provence, discovered by Belgian astronomer
Eric Elst in 1989, was named for the region where the discovering observatory is located.
Telescopes
The four main telescopes at OHP are
reflecting telescope
A reflecting telescope (also called a reflector) is a telescope that uses a single or a combination of curved mirrors that reflect light and form an image. The reflecting telescope was invented in the 17th century by Isaac Newton as an alternati ...
s with
primary mirror
A primary mirror (or primary) is the principal light-gathering surface (the objective) of a reflecting telescope.
Description
The primary mirror of a reflecting telescope is a spherical, parabolic, or hyperbolic shaped disks of polished ...
s of diameters 1.93 m, 1.52 m, 1.20 m and 0.80 m.
The 1.93 m telescope was built by
Grubb Parsons and installed at the site in 1958. One of the instruments available on the 1.93 m telescope was the high resolution
ELODIE spectrograph, replaced in 2006 by the
SOPHIE échelle spectrograph.
Michel Mayor and
Didier Queloz discovered the
planet
A planet is a large, Hydrostatic equilibrium, rounded Astronomical object, astronomical body that is generally required to be in orbit around a star, stellar remnant, or brown dwarf, and is not one itself. The Solar System has eight planets b ...
orbiting the star
51 Pegasi from observations made using ELODIE on the 1.93 m telescope. They won half of the
Nobel Prize in Physics
The Nobel Prize in Physics () is an annual award given by the Royal Swedish Academy of Sciences for those who have made the most outstanding contributions to mankind in the field of physics. It is one of the five Nobel Prizes established by the ...
2019 for this discovery.
The 1.52 m is almost identical to the 1.52 m telescope at the
European Southern Observatory
The European Organisation for Astronomical Research in the Southern Hemisphere, commonly referred to as the European Southern Observatory (ESO), is an intergovernmental organization, intergovernmental research organisation made up of 16 m ...
in
Chile
Chile, officially the Republic of Chile, is a country in western South America. It is the southernmost country in the world and the closest to Antarctica, stretching along a narrow strip of land between the Andes, Andes Mountains and the Paci ...
, and has been in use at OHP since 1967. It is predominantly used for
spectroscopic studies, using the high resolution spectrograph ''Aurélie''.
The 1.20 m telescope was the first to be installed at the site, and has been in use since 1943. It was originally installed at the
Observatoire de Paris in 1872. It is now equipped with a direct
charge-coupled device
A charge-coupled device (CCD) is an integrated circuit containing an array of linked, or coupled, capacitors. Under the control of an external circuit, each capacitor can transfer its electric charge to a neighboring capacitor. CCD sensors are a ...
(CCD) camera at the f/6 Newton focus and is mainly used for studies of variability of X-ray sources, imaging of galaxies and H II regions and astrometry of faint solar system objects.
The 0.80 m telescope was first used during site testing at nearby
Forcalquier in 1932 before the construction of the observatory, where it was later moved in 1945. The telescope is equipped with CCD cameras allowing high quality observations to be made using it, but unlike the other telescopes on site which have computer-controlled pointing systems, the 0.80 m telescope must still be pointed manually, using
setting circles. It is often used by visiting undergraduate astronomy students.
Other telescopes at OHP are operated by other organizations, including a 1 m telescope belonging to
Geneva Observatory, a 0.5 m telescope operated by the
French Space Agency for satellite tracking, and the Berlin Exoplanet Search Telescope, a 0.2 m telescope used to search for
exoplanet
An exoplanet or extrasolar planet is a planet outside the Solar System. The first confirmed detection of an exoplanet was in 1992 around a pulsar, and the first detection around a main-sequence star was in 1995. A different planet, first det ...
s by observing
transits across solar-type stars.
Geophysics
While primarily an astronomical research facility, the observatory also hosts two
geophysics
Geophysics () is a subject of natural science concerned with the physical processes and Physical property, properties of Earth and its surrounding space environment, and the use of quantitative methods for their analysis. Geophysicists conduct i ...
research stations, one studying the
mesosphere and
thermosphere, and one using
laser
A laser is a device that emits light through a process of optical amplification based on the stimulated emission of electromagnetic radiation. The word ''laser'' originated as an acronym for light amplification by stimulated emission of radi ...
s to probe the
troposphere
The troposphere is the lowest layer of the atmosphere of Earth. It contains 80% of the total mass of the Atmosphere, planetary atmosphere and 99% of the total mass of water vapor and aerosols, and is where most weather phenomena occur. From the ...
and
stratosphere
The stratosphere () is the second-lowest layer of the atmosphere of Earth, located above the troposphere and below the mesosphere. The stratosphere is composed of stratified temperature zones, with the warmer layers of air located higher ...
, studying aerosol and
ozone
Ozone () (or trioxygen) is an Inorganic compound, inorganic molecule with the chemical formula . It is a pale blue gas with a distinctively pungent smell. It is an allotrope of oxygen that is much less stable than the diatomic allotrope , break ...
content, using
lidar
Lidar (, also LIDAR, an acronym of "light detection and ranging" or "laser imaging, detection, and ranging") is a method for determining ranging, ranges by targeting an object or a surface with a laser and measuring the time for the reflected li ...
techniques.
List of discovered minor planets
The
Minor Planet Center
The Minor Planet Center (MPC) is the official body for observing and reporting on minor planets under the auspices of the International Astronomical Union (IAU). Founded in 1947, it operates at the Smithsonian Astrophysical Observatory.
Funct ...
credits the discovery of following minor planets directly to the observatory:
See also
*
List of asteroid-discovering observatories
*
List of astronomical observatories
*
*
List of observatory codes
*
Lists of telescopes
References
External links
*
*
Video about Saint-Michel Observatory available on
Paris Observatory digital library
{{Authority control
Astronomical observatories in France
Buildings and structures in Alpes-de-Haute-Provence
*
Minor-planet discovering observatories
1937 establishments in France