1063 Aquilegia, the Glossary
1063 Aquilegia, provisional designation, is a background asteroid from the inner regions of the asteroid belt, approximately 17 kilometers in diameter.[1]
Table of Contents
40 relations: Absolute magnitude, Akari (satellite), Albedo, Aquilegia, Asteroid, Asteroid belt, Asteroid family, Asteroid spectral types, Astronomical unit, Degree (angle), Ecliptic, Flora family, Flowering plant, Heidelberg-Königstuhl State Observatory, Hour, IRAS, Jet Propulsion Laboratory, Julian day, Julian year (astronomy), Karl Wilhelm Reinmuth, Kirkwood gap, Light curve, List of minor planet discoverers, Magnitude (astronomy), Minor planet, Observation arc, Orbital eccentricity, Orbital inclination, Pan-STARRS, Paul Herget, Precovery, Proper orbital elements, Richard P. Binzel, Rotation period (astronomy), S-type asteroid, Semi-major and semi-minor axes, Springer Science+Business Media, Wide-field Infrared Survey Explorer, X-type asteroid, 1054 Forsytia.
- Astronomical objects discovered in 1925
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.
Aquilegia
Aquilegia (common names: granny's bonnet, columbine) is a genus of about 130 species of perennial plants that are found in meadows, woodlands, and at higher elevations throughout the Northern Hemisphere, known for the spurred petalsPuzey, J.R., Gerbode, S.J., Hodges, S.A., Kramer, E.M., Mahadevan, L.
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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.
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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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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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Flora family
The Flora family (adj. Florian;; also known as the Ariadne family) is a prominent family of stony asteroids located in the inner region of the asteroid belt.
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Flowering plant
Flowering plants are plants that bear flowers and fruits, and form the clade Angiospermae, commonly called angiosperms.
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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.
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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).
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.
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. 1063 Aquilegia 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.
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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 minor planet discoverers
This is a list of minor-planet discoverers credited by the Minor Planet Center with the discovery of one or several minor planets (such as near-Earth and main-belt asteroids, Jupiter trojans and distant objects).
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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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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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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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Precovery
In astronomy, precovery (short for pre-discovery recovery) is the process of finding the image of an object in images or photographic plates predating its discovery, typically for the purpose of calculating a more accurate orbit.
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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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Richard P. Binzel
Richard "Rick" P. Binzel (born 1958) is an American astronomer and professor of planetary sciences at the Massachusetts Institute of Technology (MIT).
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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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S-type asteroid
S-type asteroids are asteroids with a spectral type that is indicative of a siliceous (i.e. stony) mineralogical composition, hence the name.
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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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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.
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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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X-type asteroid
The X-group of asteroids collects together several types with similar spectra, but probably quite different compositions.
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1054 Forsytia
1054 Forsytia is a dark background asteroid, approximately 46 kilometers in diameter, from the outer regions of the asteroid belt. 1063 Aquilegia and 1054 Forsytia are astronomical objects discovered in 1925, background asteroids, Discoveries by Karl Wilhelm Reinmuth, minor planet object articles (numbered) and named minor planets.
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See also
Astronomical objects discovered in 1925
- 1040 Klumpkea
- 1041 Asta
- 1042 Amazone
- 1043 Beate
- 1049 Gotho
- 1050 Meta
- 1051 Merope
- 1052 Belgica
- 1053 Vigdis
- 1054 Forsytia
- 1055 Tynka
- 1057 Wanda
- 1058 Grubba
- 1059 Mussorgskia
- 1060 Magnolia
- 1061 Paeonia
- 1062 Ljuba
- 1063 Aquilegia
- 1074 Beljawskya
- 1093 Freda
- 1283 Komsomolia
- 1328 Devota
- 1330 Spiridonia
- 1382 Gerti
- 1709 Ukraina
- 1944 Günter
- Ross 154