 Orbital diagram | |
| Discovery | |
|---|---|
| Discovered by | Johann Palisa |
| Discovery date | 19 April 1882 |
| Designations | |
| (225) Henrietta | |
| Pronunciation | /hɛnriˈɛtə/ |
Named after | Henrietta Jansen |
| A882 HA | |
| Main belt ( Cybele) | |
| Orbital characteristics [1] | |
| Epoch 31 July 2016 ( JD 2457600.5) | |
| Uncertainty parameter 0 | |
| Observation arc | 120.87 yr (44,148 d) |
| Aphelion | 4.28364 AU (640.823 Gm) |
| Perihelion | 2.4945 AU (373.17 Gm) |
| 3.38907 AU (506.998 Gm) | |
| Eccentricity | 0.26396 |
| 6.24 yr (2,278.9 d) | |
Average
orbital speed | 16.2 km/s |
| 159.155 ° | |
| 0° 9m 28.703s / day | |
| Inclination | 20.872° |
| 197.113° | |
| 104.149° | |
| Physical characteristics | |
| Dimensions | 120.49±2.5 km |
| 7.3556 h (0.30648 d) | |
| 0.0396±0.002 | |
| C | |
| 8.72 | |
225 Henrietta is a very large outer main-belt asteroid. It was discovered by Austrian astronomer Johann Palisa on April 19, 1882, in Vienna and named after Henrietta, wife of astronomer Pierre J. C. Janssen. [2] The asteroid is orbiting at a distance of 3.39 AU from the Sun with a period of 6.24 years and an eccentricity (ovalness) of 0.26. The orbital plane is inclined at an angle of 20.9° to the plane of the ecliptic. [1] 225 Henrietta belongs to Cybele group of asteroids and is probably in a 4:7 orbital resonance with the planet Jupiter. [3]
This is classified as a C-type asteroid and is probably composed of primitive carbonaceous material. It has a very dark surface, with an albedo of 0.040. Photometric measurements made from the Oakley Southern Sky Observatory during 2012 gave a light curve with a period of 7.352±0.003 h and a variation in brightness of 0.18±0.02 in magnitude. This is consistent with a synodic rotation period of 7.356±0.001 h determined in 2000. [4] In 2001, the asteroid was detected by radar from the Arecibo Observatory at a distance of 1.58 AU. The resulting data yielded an effective diameter of 128±16 km. [5]
- ^ a b "225 Henrietta". JPL Small-Body Database. NASA/ Jet Propulsion Laboratory. Retrieved 12 May 2016.
- ^ Schmadel, Lutz D. (2007). "(225) Henrietta". Dictionary of Minor Planet Names. Springer Berlin Heidelberg. p. 35. doi: 10.1007/978-3-540-29925-7_226. ISBN 978-3-540-00238-3.
- ^ Kasuga, Toshihiro; et al. (June 2012). "AKARI/AcuA Physical Studies of the Cybele Asteroid Family". The Astronomical Journal. 143 (6): 11. Bibcode: 2012AJ....143..141K. CiteSeerX 10.1.1.430.9746. doi: 10.1088/0004-6256/143/6/141. S2CID 121131179. 141.
- ^ Moravec, Patricia; Cochren, Joseph; Gerhardt, Michael; et al. (October 2012), "Asteroid Lightcurve Analysis at the Oakley Southern Sky Observatory: 2012 January-April", The Minor Planet Bulletin, 39 (4): 213–216, Bibcode: 2012MPBu...39..213M.
- ^ Magri, Christopher; et al. (January 2007), "A radar survey of main-belt asteroids: Arecibo observations of 55 objects during 1999 2003" (PDF), Icarus, 186 (1): 126–151, Bibcode: 2007Icar..186..126M, doi: 10.1016/j.icarus.2006.08.018, retrieved 14 April 2015.
- The Asteroid Orbital Elements Database
- Minor Planet Discovery Circumstances
- Asteroid Lightcurve Data File
- 225 Henrietta at AstDyS-2, Asteroids—Dynamic Site
- 225 Henrietta at the JPL Small-Body Database
