Arnold Kohlschütter
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Ernst Arnold Kohlschütter (6 July 1883 – 28 May 1969) was a German
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 ...
and astrophysicist from Halle. In 1908 he was awarded his
Ph.D. A Doctor of Philosophy (PhD, DPhil; or ) is a terminal degree that usually denotes the highest level of academic achievement in a given discipline and is awarded following a course of graduate study and original research. The name of the deg ...
from the
University of Göttingen The University of Göttingen, officially the Georg August University of Göttingen (, commonly referred to as Georgia Augusta), is a Public university, public research university in the city of Göttingen, Lower Saxony, Germany. Founded in 1734 ...
under
Karl Schwarzschild Karl Schwarzschild (; 9 October 1873 – 11 May 1916) was a German physicist and astronomer. Schwarzschild provided the first exact solution to the Einstein field equations of general relativity, for the limited case of a single spherical non-r ...
. In 1911 he began working at the
Mount Wilson observatory The Mount Wilson Observatory (MWO) is an Observatory#Astronomical observatories, astronomical observatory in Los Angeles County, California, United States. The MWO is located on Mount Wilson (California), Mount Wilson, a peak in the San Gabrie ...
, studying the spectra 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 ...
and
star A star is a luminous spheroid of plasma (physics), plasma held together by Self-gravitation, self-gravity. The List of nearest stars and brown dwarfs, nearest star to Earth is the Sun. Many other stars are visible to the naked eye at night sk ...
s in collaboration with Walter Sidney Adams. In 1914 they discovered that the absolute luminosity of a star is proportional to the relative intensity of the lines in the
spectrum A spectrum (: spectra or spectrums) is a set of related ideas, objects, or properties whose features overlap such that they blend to form a continuum. The word ''spectrum'' was first used scientifically in optics to describe the rainbow of co ...
. This allowed astronomers to determine the distance of stars, including
main sequence In astronomy, the main sequence is a classification of stars which appear on plots of stellar color index, color versus absolute magnitude, brightness as a continuous and distinctive band. Stars on this band are known as main-sequence stars or d ...
and giants, using the
spectroscope 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 ...
. He became the director of the Bonn observatory in 1925. Therein he was dedicated to astrometric studies, such as the Bonn portion of
AGK2 The ''Astronomische Gesellschaft Katalog'' (AGK) is an astrometric star catalogue of the Northern hemisphere. It was published in 3 versions from 1890 until 1975, named AGK1, AGK2 and AGK3. History Compilation for the first version, Astronomische ...
. The crater Kohlschütter on the
Moon The Moon is Earth's only natural satellite. It Orbit of the Moon, orbits around Earth at Lunar distance, an average distance of (; about 30 times Earth diameter, Earth's diameter). The Moon rotation, rotates, with a rotation period (lunar ...
is named after him.


See also

*
Ackermann–Teubner Memorial Award The Alfred Ackermann–Teubner Memorial Award for the Promotion of Mathematical Sciences recognized work in mathematical analysis. It was established in 1912 by engineer Alfred Ackermann-Teubner and was an endowment of the University of Leipzig. ...
*
Spectroscopic parallax Spectroscopic parallax or main sequence fitting is an astronomical method for measuring the distances to stars. Despite its name, it does not rely on the geometric parallax effect. The spectroscopic parallax technique can be applied to any main s ...


References


External links


Arnold Kohlschütter 6. 7. 1883-28. 5. 1969
''Astronomische Nachrichten'', vol. 292, p. 142.

1883 births 1969 deaths 20th-century German astronomers Scientists from Halle (Saale) Scientists from the Province of Saxony University of Göttingen alumni Academic staff of the University of Göttingen Academic staff of the University of Kiel Academic staff of the University of Hamburg {{Germany-astronomer-stub