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930 Westphalia, the Glossary

Index 930 Westphalia

930 Westphalia (''prov. designation'': or) is a very dark background asteroid and a slow rotator from the inner regions of the asteroid belt, that measures approximately in diameter.[1]

Table of Contents

  1. 33 relations: Absolute magnitude, Akari (satellite), Albedo, Asteroid belt, Asteroid family, Asteroid spectral types, Astronomical unit, C-type asteroid, Degree (angle), Ecliptic, Hamburg Observatory, IRAS, Jet Propulsion Laboratory, Julian day, Julian year (astronomy), Kirkwood gap, Light curve, List of slow rotators (minor planets), Magnitude (astronomy), Minor planet, Observation arc, Orbital eccentricity, Orbital inclination, Paul Herget, Photometry (astronomy), Proper orbital elements, Provisional designation in astronomy, Rotation period (astronomy), Semi-major and semi-minor axes, Simeiz Observatory, Walter Baade, Westphalia, Wide-field Infrared Survey Explorer.

  2. Astronomical objects discovered in 1920
  3. Discoveries by Walter Baade

Absolute magnitude

In astronomy, absolute magnitude is a measure of the luminosity of a celestial object on an inverse logarithmic astronomical magnitude scale.

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Akari (satellite)

AKARI (ASTRO-F) was an infrared astronomy satellite developed by Japan Aerospace Exploration Agency, in cooperation with institutes of Europe and Korea.

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Albedo

Albedo is the fraction of sunlight that is diffusely reflected by a body.

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Asteroid belt

The asteroid belt is a torus-shaped region in the Solar System, centered on the Sun and roughly spanning the space between the orbits of the planets Jupiter and Mars.

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Asteroid family

An asteroid family is a population of asteroids that share similar proper orbital elements, such as semimajor axis, eccentricity, and orbital inclination.

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Asteroid spectral types

An asteroid spectral type is assigned to asteroids based on their reflectance spectrum, color, and sometimes albedo.

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Astronomical unit

The astronomical unit (symbol: au, or AU) is a unit of length defined to be exactly equal to.

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C-type asteroid

C-type (carbonaceous) asteroids are the most common variety, forming around 75% of known asteroids.

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Degree (angle)

A degree (in full, a degree of arc, arc degree, or arcdegree), usually denoted by ° (the degree symbol), is a measurement of a plane angle in which one full rotation is 360 degrees.

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Ecliptic

The ecliptic or ecliptic plane is the orbital plane of Earth around the Sun.

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Hamburg Observatory

Hamburg Observatory (Hamburger Sternwarte) is an astronomical observatory located in the Bergedorf borough of the city of Hamburg in northern Germany.

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IRAS

The Infrared Astronomical Satellite (Dutch: Infrarood Astronomische Satelliet) (IRAS) was the first space telescope to perform a survey of the entire night sky at infrared wavelengths.

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Jet Propulsion Laboratory

Jet Propulsion Laboratory (JPL) is a Federally Funded Research and Development Center (FFRDC) in La Cañada Flintridge, California, Crescenta Valley, United States.

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Julian day

The Julian day is the continuous count of days since the beginning of the Julian period, and is used primarily by astronomers, and in software for easily calculating elapsed days between two events (e.g. food production date and sell by date).

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Julian year (astronomy)

In astronomy, a Julian year (symbol: a or aj) is a unit of measurement of time defined as exactly 365.25 days of SI seconds each.

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Kirkwood gap

A Kirkwood gap is a gap or dip in the distribution of the semi-major axes (or equivalently of the orbital periods) of the orbits of main-belt asteroids.

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Light curve

In astronomy, a light curve is a graph of the light intensity of a celestial object or region as a function of time, typically with the magnitude of light received on the y-axis and with time on the x-axis.

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List of slow rotators (minor planets)

This is a list of slow rotators—minor planets that have an exceptionally long rotation period. 930 Westphalia and list of slow rotators (minor planets) are slow rotating minor planets.

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Magnitude (astronomy)

In astronomy, magnitude is measure of the brightness of an object, usually in a defined passband.

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Minor planet

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.

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Observation arc

In observational astronomy, the observation arc (or arc length) of a Solar System body is the time period between its earliest and latest observations, used for tracing the body's path.

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Orbital eccentricity

In astrodynamics, the orbital eccentricity of an astronomical object is a dimensionless parameter that determines the amount by which its orbit around another body deviates from a perfect circle.

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Orbital inclination

Orbital inclination measures the tilt of an object's orbit around a celestial body.

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Paul Herget

Paul Herget (January 30, 1908 – August 27, 1981) was an American astronomer and director of the Cincinnati Observatory, who established the Minor Planet Center after World War II.

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Photometry (astronomy)

In astronomy, photometry, from Greek photo- ("light") and -metry ("measure"), is a technique used in astronomy that is concerned with measuring the flux or intensity of light radiated by astronomical objects.

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Proper orbital elements

The proper orbital elements or proper elements of an orbit are constants of motion of an object in space that remain practically unchanged over an astronomically long timescale.

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Provisional designation in astronomy

Provisional designation in astronomy is the naming convention applied to astronomical objects immediately following their discovery.

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Rotation period (astronomy)

In astronomy, the rotation period or spin period of a celestial object (e.g., star, planet, moon, asteroid) has two definitions.

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Semi-major and semi-minor axes

In geometry, the major axis of an ellipse is its longest diameter: a line segment that runs through the center and both foci, with ends at the two most widely separated points of the perimeter.

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Simeiz Observatory

Simeiz Observatory (also spelled Simeis or Simeïs) was an astronomy research observatory until the mid-1950s.

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Walter Baade

Wilhelm Heinrich Walter Baade (March 24, 1893 – June 25, 1960) was a German astronomer who worked in the United States from 1931 to 1959. 930 Westphalia and Walter Baade are Discoveries by Walter Baade.

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Westphalia

Westphalia (Westfalen; Westfalen) is a region of northwestern Germany and one of the three historic parts of the state of North Rhine-Westphalia.

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Wide-field Infrared Survey Explorer

Wide-field Infrared Survey Explorer (WISE, observatory code C51, Explorer 92 and MIDEX-6) is a NASA infrared astronomy space telescope in the Explorers Program launched in December 2009.

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See also

Astronomical objects discovered in 1920

Discoveries by Walter Baade

References

[1] https://en.wikipedia.org/wiki/930_Westphalia