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26 relations: Asteroid belt, Asteroid family, Asteroid spectral types, Astronomical unit, Degree (angle), Kirkwood gap, Kiyotsugu Hirayama, List of minor planets: 2001–3000, Orbital eccentricity, Orbital inclination, Parent body, S-type asteroid, Semi-major and semi-minor axes, 1158 Luda, 1215 Boyer, 170 Maria, 292 Ludovica, 3066 McFadden, 472 Roma, 652 Jubilatrix, 695 Bella, 714 Ulula, 787 Moskva, 875 Nymphe, 879 Ricarda, 897 Lysistrata.
Asteroid belt
The asteroid belt is the circumstellar disc in the Solar System located roughly between the orbits of the planets Mars and Jupiter.
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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 emission spectrum, color, and sometimes albedo (reflectivity).
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Astronomical unit
The astronomical unit (symbol: au, ua, or AU) is a unit of length, roughly the distance from Earth to the Sun.
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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, defined so that a full rotation is 360 degrees.
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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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Kiyotsugu Hirayama
was a Japanese astronomer, best known for his discovery that many asteroid orbits were more similar to one another than chance would allow, leading to the concept of asteroid families, now called "Hirayama families" in his honour.
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List of minor planets: 2001–3000
#FA8072 | 2078 Nanking || 1975 AD || January 12, 1975 || Nanking || Purple Mountain Obs.
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Orbital eccentricity
The orbital eccentricity of an astronomical object is a 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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Parent body
In meteoritics, a parent body is the celestial body from which originates a meteorite or a class of meteorites.
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S-type asteroid
S-type asteroids are asteroids with a spectral type that is indicative of a silicaceous (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 widest points of the perimeter.
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1158 Luda
1158 Luda, provisional designation, is a stony asteroid from the middle regions of the asteroid belt, approximately 19 kilometers in diameter.
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1215 Boyer
1215 Boyer, provisional designation, is a stony Eunomian asteroid from the central region of the asteroid belt, approximately 20 kilometers in diameter.
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170 Maria
170 Maria is a Main belt asteroid that was discovered by French astronomer Henri Joseph Perrotin on January 10, 1877.
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292 Ludovica
292 Ludovica is a Main belt asteroid.
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3066 McFadden
3066 McFadden, provisional designation, is a stony background asteroid from the central regions of the asteroid belt, approximately in diameter.
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472 Roma
472 Roma is an asteroid.
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652 Jubilatrix
652 Jubilatrix is a minor planet orbiting the Sun.
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695 Bella
695 Bella is a minor planet orbiting the Sun.
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714 Ulula
714 Ulula is a minor planet orbiting the Sun.
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787 Moskva
787 Moskva is a minor planet orbiting the Sun.
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875 Nymphe
875 Nymphe is a minor planet orbiting the Sun.
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879 Ricarda
879 Ricarda is a minor planet orbiting the Sun that was discovered by German astronomer Max Wolf on July 22, 1917.
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897 Lysistrata
897 Lysistrata is a minor planet orbiting the Sun that was discovered by German astronomer Max Wolf on August 3, 1918.
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Redirects here:
Maria asteroid, Maria asteroids, Roma family.
References
[1] https://en.wikipedia.org/wiki/Maria_family
