Discovery | |
---|---|
Discovered by | G. Witt |
Discovery date | 8 October 1896 |
Designations | |
(422) Berolina | |
Pronunciation | /bɛrəˈlaɪnə/ |
Named after | Berlin |
1896 DA | |
Main belt | |
Orbital characteristics [1] | |
Epoch 31 July 2016 (JD 2457600.5) | |
Uncertainty parameter 0 | |
Observation arc | 109.00 yr (39811 d) |
Aphelion | 2.70724 AU (404.997 Gm) |
Perihelion | 1.74907 AU (261.657 Gm) |
2.22815 AU (333.326 Gm) | |
Eccentricity | 0.21502 |
3.33 yr (1214.8 d) | |
29.4528° | |
0° 17m 46.817s / day | |
Inclination | 4.99913° |
9.08604° | |
335.361° | |
Physical characteristics | |
Dimensions | 10.714 km |
12.79 h (0.533 d) | |
10.83 | |
422 Berolina is a typical Main belt asteroid.
It was discovered by G. Witt on 8 October 1896 in Berlin. It was first of his two asteroid discoveries. The other was the famous asteroid 433 Eros.
Although it has an orbit similar to the Flora family asteroids, it appears to be an unrelated interloper due to not being of the S spectral type (see the PDS asteroid taxonomy data set).
366 Vincentina is a fairly large main belt asteroid.
263 Dresda is a typical Main belt asteroid. It belongs to the Koronis family of asteroids.
303 Josephina is a large Main belt asteroid. It was discovered by Elia Millosevich on 12 February 1891 in Rome. It was first of his two asteroid discoveries. The other was 306 Unitas.
396 Aeolia is a typical main belt asteroid. It was discovered by the French astronomer Auguste Charlois on 1 December 1894 from Nice, and may have been named for the ancient land of Aeolis. The asteroid is orbiting the Sun at a distance of 2.74 AU with a period of 4.54 years and an eccentricity (ovalness) of 0.16. The orbital plane is inclined at an angle of 2.5° to the plane of the ecliptic. This is the largest member of the eponymously named Aeolia asteroid family, a small group of asteroids with similar orbits that have an estimated age of less than 100 million years.
410 Chloris is a very large main-belt asteroid that was discovered by Auguste Charlois on January 7, 1896, in Nice. It is classified as a C-type asteroid and is probably composed of primitive carbonaceous material. The spectrum of the asteroid displays evidence of aqueous alteration. It is the namesake of the Chloris family of asteroids.
411 Xanthe is an asteroid from the outer regions of the asteroid belt, approximately 77 kilometers in diameter. It was discovered by French astronomer Auguste Charlois at Nice Observatory on 7 January 1896. The asteroid was named after Xanthe, an Oceanid or sea nymph, and one of the many Titan daughters of Oceanus and Tethys from Greek mythology.
414 Liriope is a large Main belt asteroid. It is classified as a C-type asteroid and is probably composed of carbonaceous material.
415 Palatia is a large main belt asteroid that was discovered by German astronomer Max Wolf on 7 February 1896 in Heidelberg.
416 Vaticana is a large main belt asteroid.
417 Suevia is a typical Main belt asteroid. It is classified as a K-type/S-type asteroid.
420 Bertholda is a very large main-belt asteroid. It was discovered by Max Wolf on September 7, 1896, in Heidelberg, Germany. The object is part of the Cybele asteroid group, and is classified as a P-type asteroid.
421 Zähringia, provisional designation 1896 CZ, is a stony asteroid from the intermediate asteroid belt, approximately 14 kilometers in diameter. It was discovered on 7 September 1896, by astronomer Max Wolf at Heidelberg Observatory in Germany. The asteroid was named for the House of Zähringen, a medieval noble family that ruled parts of Swabia and Switzerland.
424 Gratia is a large Main belt asteroid.
425 Cornelia is a large Main belt asteroid. It was discovered by Auguste Charlois on 28 December 1896 in Nice. It is named after Cornelia Africana.
443 Photographica is a typical Main belt asteroid. It is classified as an S-type asteroid.
534 Nassovia is a minor planet orbiting the Sun. It is a member of the Koronis family of asteroids.
633 Zelima is a minor planet orbiting the Sun in the asteroid belt with a magnitude of 10.7. The name may have been inspired by the asteroid's provisional designation 1907 ZM.
668 Dora is an asteroid orbiting in the asteroid belt located roughly between the orbits of the planets Mars and Jupiter. The name may have been inspired by the asteroid's provisional designation 1908 DO.
768 Struveana is a minor planet orbiting the Sun. The asteroid was named jointly in honor of Baltic German astronomers Friedrich Georg Wilhelm von Struve, Otto Wilhelm von Struve and Karl Hermann Struve.
901 Brunsia is an S-type asteroid belonging to the Flora family in the Main Belt. Its rotation period is 3.136 hours.