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1144 Oda

Index 1144 Oda

1144 Oda, provisional designation, is a dark Hildian asteroid from the outermost regions of the asteroid belt, approximately 57 kilometers in diameter. [1]

Table of Contents

  1. 39 relations: Absolute magnitude, Akari (satellite), Albedo, Asteroid, Asteroid belt, Asteroid family, Asteroid spectral types, Astronomical unit, Calendar (stationery), D-type asteroid, Degree (angle), Ecliptic, Geneva Observatory, Heidelberg-Königstuhl State Observatory, Hilda asteroid, Hilda family, Hour, Ingrid van Houten-Groeneveld, IRAS, Jet Propulsion Laboratory, Julian day, Julian year (astronomy), Karl Wilhelm Reinmuth, Kirkwood gap, Light curve, List of slow rotators (minor planets), Magnitude (astronomy), Minor planet, Observation arc, Orbital eccentricity, Orbital inclination, Orbital resonance, Palomar Transient Factory, Pan-STARRS, Rotation period (astronomy), Semi-major and semi-minor axes, Springer Science+Business Media, Wide-field Infrared Survey Explorer, X-type asteroid.

  2. Astronomical objects discovered in 1930
  3. D-type asteroids (Tholen)
  4. Hilda asteroids

Absolute magnitude

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

See 1144 Oda and Absolute magnitude

Akari (satellite)

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

See 1144 Oda and Akari (satellite)

Albedo

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

See 1144 Oda and Albedo

Asteroid

An asteroid is a minor planet—an object that is neither a true planet nor an identified comet— that orbits within the inner Solar System.

See 1144 Oda and Asteroid

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.

See 1144 Oda and Asteroid belt

Asteroid family

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

See 1144 Oda and Asteroid family

Asteroid spectral types

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

See 1144 Oda and Asteroid spectral types

Astronomical unit

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

See 1144 Oda and Astronomical unit

Calendar (stationery)

A calendar is used to display dates and related information, usually in a table format.

See 1144 Oda and Calendar (stationery)

D-type asteroid

D-type asteroids have a very low albedo and a featureless reddish spectrum.

See 1144 Oda and D-type asteroid

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.

See 1144 Oda and Ecliptic

Geneva Observatory

The Geneva Observatory (Observatoire de Genève, Observatorium von Genf) is an astronomical observatory at Sauverny (CH) in the municipality of Versoix, Canton of Geneva, in Switzerland.

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Heidelberg-Königstuhl State Observatory

Heidelberg-Königstuhl State Observatory (Landessternwarte Heidelberg-Königstuhl) is a historic astronomical observatory located near the summit of the Königstuhl hill in the city of Heidelberg in Germany.

See 1144 Oda and Heidelberg-Königstuhl State Observatory

Hilda asteroid

The Hilda asteroids (adj. Hildian) are a dynamical group of more than 5,000 asteroids located beyond the asteroid belt but within Jupiter's orbit, in a 3:2 orbital resonance with Jupiter. 1144 Oda and Hilda asteroid are Hilda asteroids.

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Hilda family

The Hilda family (001) is an ancient collisional asteroid family of at least 409 known asteroids, named for its largest member, the -across asteroid 153 Hilda. 1144 Oda and Hilda family are Hilda asteroids.

See 1144 Oda and Hilda family

Hour

An hour (symbol: h; also abbreviated hr) is a unit of time historically reckoned as of a day and defined contemporarily as exactly 3,600 seconds (SI).

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Ingrid van Houten-Groeneveld

Ingrid van Houten-Groeneveld (21 October 1921 – 30 March 2015) was a Dutch astronomer.

See 1144 Oda and Ingrid van Houten-Groeneveld

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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Karl Wilhelm Reinmuth

Karl Wilhelm Reinmuth (4 April 1892 in Heidelberg – 6 May 1979 in Heidelberg) was a German astronomer and a prolific discoverer of 395 minor planets. 1144 Oda and Karl Wilhelm Reinmuth are Discoveries by Karl Wilhelm Reinmuth.

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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.

See 1144 Oda and Kirkwood gap

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.

See 1144 Oda and Light curve

List of slow rotators (minor planets)

This is a list of slow rotators—minor planets that have an exceptionally long rotation period.

See 1144 Oda and List of slow rotators (minor planets)

Magnitude (astronomy)

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

See 1144 Oda and Magnitude (astronomy)

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.

See 1144 Oda and Minor planet

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.

See 1144 Oda and Observation arc

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.

See 1144 Oda and Orbital eccentricity

Orbital inclination

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

See 1144 Oda and Orbital inclination

Orbital resonance

In celestial mechanics, orbital resonance occurs when orbiting bodies exert regular, periodic gravitational influence on each other, usually because their orbital periods are related by a ratio of small integers.

See 1144 Oda and Orbital resonance

Palomar Transient Factory

The Palomar Transient Factory (PTF, obs. code: I41), was an astronomical survey using a wide-field survey camera designed to search for optical transient and variable sources such as variable stars, supernovae, asteroids and comets.

See 1144 Oda and Palomar Transient Factory

Pan-STARRS

The Panoramic Survey Telescope and Rapid Response System (Pan-STARRS1; obs. code: F51 and Pan-STARRS2 obs. code: F52) located at Haleakala Observatory, Hawaii, US, consists of astronomical cameras, telescopes and a computing facility that is surveying the sky for moving or variable objects on a continual basis, and also producing accurate astrometry and photometry of already-detected objects.

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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.

See 1144 Oda and Rotation period (astronomy)

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.

See 1144 Oda and Semi-major and semi-minor axes

Springer Science+Business Media

Springer Science+Business Media, commonly known as Springer, is a German multinational publishing company of books, e-books and peer-reviewed journals in science, humanities, technical and medical (STM) publishing.

See 1144 Oda and Springer Science+Business Media

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.

See 1144 Oda and Wide-field Infrared Survey Explorer

X-type asteroid

The X-group of asteroids collects together several types with similar spectra, but probably quite different compositions.

See 1144 Oda and X-type asteroid

See also

Astronomical objects discovered in 1930

D-type asteroids (Tholen)

Hilda asteroids

References

[1] https://en.wikipedia.org/wiki/1144_Oda