1372 Haremari
| 1372 Haremari | |
| Upptäckt[1] | |
|---|---|
| Upptäckare | K. Reinmuth |
| Upptäcktsplats | Heidelberg |
| Upptäcktsdatum | 31 augusti 1935 |
| Beteckningar | |
| MPC-beteckning | (1372) Haremari |
| Alternativnamn | 1935 QK, 1928 DX, 1937 BD, 1944 QK, 1951 EW1, 1953 OM, 1953 PZ[1] |
| Småplanetskategori | Asteroidbältet Watsonia-asteroid[2] |
| Omloppsbana[3] | |
| Epok: 21 januari 2022 | |
| Aphelium | 3,177 AU |
| Perihelium | 2,353 AU |
| Halv storaxel | 2,765 AU |
| Excentricitet | 0,1489441 |
| Siderisk omloppstid | 4,6 år |
| Medelomloppshastighet | 17,91 km/s |
| Medelanomali | 227,1° |
| Inklination | 16,45° |
| Longitud för uppstigande nod | 327,4° |
| Periheliumargument | 88,09° |
| Fysikaliska data[1] | |
| Diameter | 26,4 km |
| Synodisk rotationsperiod | 15,2 h |
| Albedo | 0,039 |
| Absolut magnitud (H) | 11,21[3] |
| Hitta fler artiklar om astronomi med | |
1372 Haremari eller 1935 QK[1] är en asteroid i huvudbältet, som upptäcktes 31 augusti 1935 av den tyske astronomen Karl Wilhelm Reinmuth i Heidelberg. Den har fått sitt namn efter en kvinna vid Ruprecht-Karls-Universität Heidelberg.[4]
Asteroiden har en diameter på ungefär 26 kilometer och den tillhör asteroidgruppen Watsonia.[2]
Asteroiden kan vara en trojan till dvärgplaneten Ceres.
Referenser
- ^ [a b c d] ”JPL Small-Body Database Browser 1372 Haremari” (på engelska). Solar System Dynamics. NASA/Jet Propulsion Laboratory. https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=1372. Läst 13 juni 2017.
- ^ [a b] ”AstDyS 1372 Haremari” (på engelska). https://newton.spacedys.com/astdys/index.php?pc=1.1.6&n=1372. Läst 21 augusti 2020.
- ^ [a b] Minor Planet Center Queries, uppdaterad 29 januari 2022.
- ^ Schmadel, Lutz D. (2003). Dictionary of Minor Planet Names – (1372) Haremari. Springer Berlin Heidelberg. sid. 111. ISBN 978-3-540-29925-7. https://link.springer.com/referenceworkentry/10.1007/978-3-540-29925-7_1373. Läst 13 juni 2017
| |||||||||||
| ||||||||||||||||||||||||||||||||||||||
Media som används på denna webbplats
PIA19547: Ceres RC3 Animation - Still Frame 25
http://photojournal.jpl.nasa.gov/catalog/PIA19547
http://www.jpl.nasa.gov/news/news.php?feature=4582
UPLOADER NOTE: Frame 25 of the original GIF animation (16.096KB) - via JASC Animation Shop v 2.02.
In this closest-yet view of Ceres, the brightest spots within a crater in the northern hemisphere are revealed to be composed of many smaller spots. This frame is from an animation of sequences taken by NASA's Dawn spacecraft on May 4, 2015.
This animation shows a sequence of images taken by NASA's Dawn spacecraft on May 4, 2015, from a distance of 8,400 miles (13,600 kilometers), in its RC3 mapping orbit. The image resolution is 0.8 mile (1.3 kilometers) per pixel.
In this closest-yet view, the brightest spots within a crater in the northern hemisphere are revealed to be composed of many smaller spots. However, their exact nature remains unknown.
Dawn's mission is managed by JPL for NASA's Science Mission Directorate in Washington. Dawn is a project of the directorate's Discovery Program, managed by NASA's Marshall Space Flight Center in Huntsville, Alabama. UCLA is responsible for overall Dawn mission science. Orbital ATK, Inc., in Dulles, Virginia, designed and built the spacecraft. The German Aerospace Center, the Max Planck Institute for Solar System Research, the Italian Space Agency and the Italian National Astrophysical Institute are international partners on the mission team. For a complete list of acknowledgements, visit http://dawn.jpl.nasa.gov/mission.
For more information about the Dawn mission, visit http://dawn.jpl.nasa.gov.
A cluster of mysterious bright spots on dwarf planet Ceres can be seen in this image, taken by NASA's Dawn spacecraft from an altitude of 2,700 miles (4,400 kilometers). The image, with a resolution of 1,400 feet (410 meters) per pixel, was taken on June 9, 2015.