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The Valz Prize ''(Prix Valz)'' was awarded by the
French Academy of Sciences The French Academy of Sciences (, ) is a learned society, founded in 1666 by Louis XIV at the suggestion of Jean-Baptiste Colbert, to encourage and protect the spirit of French Scientific method, scientific research. It was at the forefron ...
, from 1877 through 1970, to honor advances in
astronomy Astronomy is a natural science that studies celestial objects and the phenomena that occur in the cosmos. It uses mathematics, physics, and chemistry in order to explain their origin and their overall evolution. Objects of interest includ ...
.


History

The Valz Prize was established in June 1874 when the widow of astronomer Benjamin Valz, Marie Madeleine Julie Malhian, donated 10,000
francs The franc is any of various units of currency. One franc is typically divided into 100 centimes. The name is said to derive from the Latin inscription ''francorum rex'' ( King of the Franks) used on early French coins and until the 18th centur ...
to establish a prize in honor of her late husband. The Valz Prize was to be awarded for work of similar stature as that honored by the pre-existing
Lalande Prize The Lalande Prize (French: ''Prix Lalande'' also known as Lalande Medal) was an award for scientific advances in astronomy, given from 1802 until 1970 by the French Academy of Sciences. The prize was endowed by astronomer Jérôme Lalande in 1801 ...
. The first Valz Prize was awarded in 1877 to brothers Paul and Prosper Henry, and was for the sum of 460 francs. Save for 1924, the French Academy of Sciences awarded the Valz Prize annually from 1877 to 1943. After 1943, the prize was awarded only sporadically (only once per decade from 1950 to 1970). In 1970, the Valz Prize was combined with the
Lalande Prize The Lalande Prize (French: ''Prix Lalande'' also known as Lalande Medal) was an award for scientific advances in astronomy, given from 1802 until 1970 by the French Academy of Sciences. The prize was endowed by astronomer Jérôme Lalande in 1801 ...
to create the Lalande-Valz Prize, which continued to be awarded through 1996. In 1997, that prize was combined with numerous other Academy prizes to create the Grande Médaille.


List of Valz Prize winners

* 1877 – Paul Henry and Prosper Henry (joint award) – Charts to facilitate search for
minor planets According to the International Astronomical Union (IAU), a minor planet is an astronomical object in direct orbit around the Sun that is exclusively classified as neither a planet nor a comet. Before 2006, the IAU officially used the term ''minor ...
* 1878 – Julius Schmidt – Selenographic work * 1879 – Étienne Trouvelot – Work on
Jupiter Jupiter is the fifth planet from the Sun and the List of Solar System objects by size, largest in the Solar System. It is a gas giant with a Jupiter mass, mass more than 2.5 times that of all the other planets in the Solar System combined a ...
,
Saturn Saturn is the sixth planet from the Sun and the second largest in the Solar System, after Jupiter. It is a gas giant, with an average radius of about 9 times that of Earth. It has an eighth the average density of Earth, but is over 95 tim ...
, and
Mars Mars is the fourth planet from the Sun. It is also known as the "Red Planet", because of its orange-red appearance. Mars is a desert-like rocky planet with a tenuous carbon dioxide () atmosphere. At the average surface level the atmosph ...
* 1880 –
Wilhelm Tempel Ernst Wilhelm Leberecht Tempel (4 December 1821 – 16 March 1889), normally known as Wilhelm Tempel, was a German astronomer who worked in Marseille until the outbreak of the Franco-Prussian War in 1870, then later moved to Italy. Tempel was b ...
– Discovery of twenty
comets A comet is an icy, small Solar System body that warms and begins to release gases when passing close to the Sun, a process called outgassing. This produces an extended, gravitationally unbound atmosphere or coma surrounding the nucleus, an ...
* 1881 – David Gill – Work on the determination of the
parallax Parallax is a displacement or difference in the apparent position of an object viewed along two different sightline, lines of sight and is measured by the angle or half-angle of inclination between those two lines. Due to perspective (graphica ...
of the
Sun The Sun is the star at the centre of the Solar System. It is a massive, nearly perfect sphere of hot plasma, heated to incandescence by nuclear fusion reactions in its core, radiating the energy from its surface mainly as visible light a ...
* 1882 – William Huggins – Applications of photography to the study of the spectra of celestial bodies * 1882 – Luiz Cruls – Spectral studies of the Great Comet of 1882 * 1883 –
Édouard Jean-Marie Stephan Édouard is both a French given name and a surname, equivalent to Edward in English. Notable people with the name include: * Édouard Balladur (born 1929), French politician * Édouard Boubat (1923–1999), French photographer * Édouard Colonne (1 ...
– Discoveries of
nebula A nebula (; or nebulas) is a distinct luminescent part of interstellar medium, which can consist of ionized, neutral, or molecular hydrogen and also cosmic dust. Nebulae are often star-forming regions, such as in the Pillars of Creation in ...
e * 1884 – Friedrich Karl Ginzel – Work on the eclipses of the Sun * 1885 – Friedrich Wilhelm Gustav Spörer – Work on
sunspots Sunspots are temporary spots on the Sun's surface that are darker than the surrounding area. They are one of the most recognizable Solar phenomena and despite the fact that they are mostly visible in the solar photosphere they usually affe ...
* 1886 – Camille Guillaume Bigourdan – Research on the problem of personal error * 1887 – Ernest Perigaud – Investigation of the meridian instruments of the
Paris Observatory The Paris Observatory (, ), a research institution of the Paris Sciences et Lettres University, is the foremost astronomical observatory of France, and one of the largest astronomical centres in the world. Its historic building is on the Left Ban ...
* 1888 –
Edward Charles Pickering Edward Charles Pickering (July 19, 1846 – February 3, 1919) was an American astronomer and physicist and the older brother of William Henry Pickering. Along with Carl Vogel, Pickering discovered the first spectroscopic binary stars. He wrote ' ...
– Photometric work on stellar magnitude * 1889 –
Auguste Charlois Auguste Honoré Charlois (; November 26, 1864 – March 26, 1910) was a French astronomer who discovered 99 asteroids while working at the Nice Observatory in southeastern France. Asteroid discovery His first discovery was the asteroid 267 Tirz ...
– Astronomical work on orbits of seven
asteroids An asteroid is a minor planet—an object larger than a meteoroid that is neither a planet nor an identified comet—that orbits within the Solar System#Inner Solar System, inner Solar System or is co-orbital with Jupiter (Trojan asteroids). As ...
* 1890 – S. de Glasenapp – Study on the
double star In observational astronomy, a double star or visual double is a pair of stars that appear close to each other as viewed from Earth, especially with the aid of optical telescopes. This occurs because the pair either forms a binary star (i.e. a ...
s appearing in the
Pulkovo Pulkovo may refer to: *Pulkovo Heights marking the southern limit of Saint Petersburg, Russia *Pulkovo Airport serving Saint Petersburg, Russia * Pulkovo Aviation Enterprise, a former (until 2006) state airline based in Saint Petersburg, Russia *Pu ...
Catalog * 1891 –
Hermann Carl Vogel Hermann Carl Vogel (; ; 3 April 1841 – 13 August 1907) was a German astrophysicist. He was born in Leipzig, Kingdom of Saxony. From 1882 to 1907 he was director of the Astrophysical Observatory, Potsdam. He made extensive discoveries ...
– Research in
spectroscopy Spectroscopy is the field of study that measures and interprets electromagnetic spectra. In narrower contexts, spectroscopy is the precise study of color as generalized from visible light to all bands of the electromagnetic spectrum. Spectro ...
* 1892 – Pierre Puiseux – Entirety of his work, including that on the constant of aberration * 1893 –
Adolf Berberich Adolf Joseph Berberich (16 November 1861 – 27 April 1920) was a German astronomer best known for his work on calculating the orbits of minor planets and double stars. The minor planet 776 Berbericia was named in his honour. Early life Adolf ...
– Calculations of orbits of double stars, comets, and
planets A planet is a large, rounded 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 by the most restrictive definition of the te ...
* 1894 – Jean Coniel – Calculations of asteroid orbits * 1895 – William Frederick Denning – Work on
meteors A meteor, known colloquially as a shooting star, is a glowing streak of a small body (usually meteoroid) going through Earth's atmosphere, after being heated to incandescence by collisions with air molecules in the upper atmosphere, creating a ...
and discoveries of comets * 1896 – Joseph Bossert – Catalog of 3,950 stars * 1897 – Louis Fabry – Research on orbits of comets * 1898 – Élie Colin – Research on astronomy and
geodesy Geodesy or geodetics is the science of measuring and representing the Figure of the Earth, geometry, Gravity of Earth, gravity, and Earth's rotation, spatial orientation of the Earth in Relative change, temporally varying Three-dimensional spac ...
, especially
latitude In geography, latitude is a geographic coordinate system, geographic coordinate that specifies the north-south position of a point on the surface of the Earth or another celestial body. Latitude is given as an angle that ranges from −90° at t ...
* 1899 – Magnus Nyrén – Sidereal astronomy and observations on the meridian * 1900 – Aloys Verschaffel – Meridian observations and catalog * 1901 – Charles André – Treatise o
''Traite d'Astronomie Stellaire''
ref name=English1902>
* 1902 – Ernst Hartwig –
Heliometer A heliometer (from Greek ἥλιος ''hḗlios'' "sun" and ''measure'') is an instrument originally designed for measuring the variation of the Sun's diameter at different seasons of the year, but applied now to the modern form of the instrumen ...
observations and work on
variable stars A variable star is a star whose brightness as seen from Earth (its apparent magnitude) changes systematically with time. This variation may be caused by a change in emitted light or by something partly blocking the light, so variable stars are ...
* 1903 – Alphonse Borrelly – Discoveries of comets * 1904 – Campos Rodrigues – Determination of solar parallax by means of the asteroid
Eros Eros (, ; ) is the Greek god of love and sex. The Romans referred to him as Cupid or Amor. In the earliest account, he is a primordial god, while in later accounts he is the child of Aphrodite. He is usually presented as a handsome young ma ...
* 1905 – Michel Giacobini – discovery of ten comets * 1906 –
Johann Palisa Johann Palisa (6 December 1848 – 2 May 1925) was an Austrian astronomer, born in Troppau, Austrian Silesia, now Czech Republic. He was a prolific discoverer of asteroids, discovering 122 in all, from 136 Austria in 1874 to 1073 G ...
– Entirety of his astronomical research * 1907 – Michel Giacobini – Astronomical work * 1908 – Michel Luizet – Work on variable stars * 1909 – Aymar de la Baume Pluvinel – Entirety of his astronomical work * 1910 – Stéphane Javelle – Works on nebulae and comets * 1911 – Charlemagne Rambaud – Astronomical work * 1912 – Alexandre Schaumasse – Comet discoveries * 1913 –
Alfred Fowler Alfred Fowler, CBE FRS (22 March 1868, in Yorkshire – 24 June 1940) was an English astronomer and spectroscopist. Early life and career He was born in Wilsden on the outskirts of Bradford, Yorkshire and educated at London's Norma ...
– Work on the principal series of hydrogen lines * 1914 – Pierre Salet – Research on polarization phenomena * 1914 – Stanislas Chevalier – Research on the Sun * 1915 – Armand Lambert – Work as an observer and in
applied mathematics Applied mathematics is the application of mathematics, mathematical methods by different fields such as physics, engineering, medicine, biology, finance, business, computer science, and Industrial sector, industry. Thus, applied mathematics is a ...
* 1916 – Giovanni Boccardi – Research on variation of latitude; discovery of a sensible inequality in the semi-lunar period * 1917 – Alexandre Schaumasse – Discovery of comet 1917b (C/1917 H1) * 1918 –
Frédéric Sy Frédéric Sy (1861-1917) was a French astronomer and a discoverer of minor planets. He worked at the Paris Observatory from 1879 to 1887, and as the assistant astronomer at the Algiers Observatory, North Africa, from 1887 to 1918. While workin ...
– Entirety of his astronomical work * 1919 – Felix Boquet – Entirety of his scientific work * 1920 – Ernest Maubant – Calculation of perturbations of Tempel-Swift Comet * 1921 – Jean Trousset – Research on double stars, the errors of divided circles, and studies of Jupiter's moon, Pasiphae * 1922 – Jean François Chazy – Papers on the
three-body problem In physics, specifically classical mechanics, the three-body problem is to take the initial positions and velocities (or momenta) of three point masses orbiting each other in space and then calculate their subsequent trajectories using Newton' ...
* 1923 –
Walter Sydney Adams Walter Sydney Adams (December 20, 1876 – May 11, 1956) was an American astronomer. He is renowned for his pioneering work in spectroscopy. Life and work Adams was born in Antioch, Ottoman Empire, to Lucien Harper Adams and Nancy Dorrance ...
– Work on Solar and stellar spectroscopy * 1924 – no award * 1925 – Vojislav Michkovitch (or Vojislav Mišković) – Work on Stellar statistics * 1926 – Frank Schlesinger – Astronomical work, especially for work on the
stellar parallax Stellar parallax is the apparent shift of position (''parallax'') of any nearby star (or other object) against the background of distant stars. By extension, it is a method for determining the distance to the star through trigonometry, the stel ...
* 1927 – Lucien d'Azambuja – Work on sunspots,
solar flares A solar flare is a relatively intense, localized emission of electromagnetic radiation in the Stellar atmosphere, Sun's atmosphere. Flares occur in active regions and are often, but not always, accompanied by coronal mass ejections, solar partic ...
, and the solar chromosphere * 1928 – George Van Biesbroeck – Entirety of his astronomical work * 1929 – Louis Dominique Joseph Armand Dunoyer de Segonzac – Research on
spirit level A spirit level, bubble level, or simply a level, is an Measuring instrument, instrument designed to indicate whether a surface is Horizontal plane, horizontal (level) or vertical direction, vertical (plumb-bob, plumb). Two basic designs exis ...
s and on
photoelectric cells A solar cell, also known as a photovoltaic cell (PV cell), is an electronic device that converts the energy of light directly into electricity by means of the photovoltaic effect.
* 1930 – Gilbert Rougier – Work on photoelectric cells * 1931 – Henri Chretien – Invention of the
anamorphic Anamorphic format is a cinematography technique that captures widescreen images using recording media with narrower native Aspect ratio (image), aspect ratios. Originally developed for 35 mm movie film, 35 mm film to create widescreen pres ...
lens * 1932 – Jean Dufay – Work on astronomical photometry * 1933 – Henri Labrouste – Research into periodic solar phenomena * 1934 – Ferdinand Quenisset – Observations on comets * 1935 – Raymond Tremblot – For the entirety of his astronomical work * 1936 –
André Couder André Couder (27 November 1897 – 16 January 1979) was a French optician and astronomer. Information From 1925, he worked in the optics laboratory of the Paris Observatory. Between 1952 and 1958 he was vice-president of the International Astrono ...
– Work on optical instruments * 1937 – Maurice Burgaud – Work in
Shanghai Shanghai, Shanghainese: , Standard Chinese pronunciation: is a direct-administered municipality and the most populous urban area in China. The city is located on the Chinese shoreline on the southern estuary of the Yangtze River, with the ...
,
China China, officially the People's Republic of China (PRC), is a country in East Asia. With population of China, a population exceeding 1.4 billion, it is the list of countries by population (United Nations), second-most populous country after ...
on
terrestrial magnetism The ''Journal of Geophysical Research'' is a peer-reviewed scientific journal. It is the flagship journal of the American Geophysical Union. It contains original research on the physical, chemical, and biological processes that contribute to the u ...
* 1938 – Pierre Lacroute – Work in physical astronomy * 1938 – Rene Bernard – Work in "the light of the night sky" * 1940 – Jeanne Clavier – Work on a photographic map of the heavens * 1941 – Junior Gauzit – Research in physical astronomy * 1942 – Jean Rösch – Work in physical astronomy * 1943 – Rose Sainturier (née Rose Bonnet) – Work on double stars * 1944-1945 – Not awarded * 1946 – Raoul Goudey – Work on
gravity In physics, gravity (), also known as gravitation or a gravitational interaction, is a fundamental interaction, a mutual attraction between all massive particles. On Earth, gravity takes a slightly different meaning: the observed force b ...
* 1947-1948 – Not awarded * 1949 – Jean Delhaye – Work in stellar statistics * 1950-1958 – Not awarded * 1959 – Fernan Nahon – Work on stellar statistics and dynamics * 1960-1968 – Not awardedNo documentation can be found for 1966 and 1967. * 1969 – André Baranne – Work on optical astronomy * 1970 – Not awarded


Notes


See also

* List of astronomy awards


References

{{Reflist, colwidth=30em Awards of the French Academy of Sciences Astronomy prizes 1874 establishments in France Awards established in 1874