Astronomy:127 Johanna
![]() A three-dimensional model of 127 Johanna based on its light curve | |
Discovery | |
---|---|
Discovered by | Paul Henry and Prosper Henry |
Discovery date | 5 November 1872 |
Designations | |
(127) Johanna | |
Pronunciation | /dʒoʊˈhænə/[1] |
Named after | Joan of Arc |
A872 VB | |
Minor planet category | Main belt |
Orbital characteristics[2] | |
Epoch 31 July 2016 (JD 2457600.5) | |
Uncertainty parameter 0 | |
Observation arc | 98.53 yr (35989 d) |
|{{{apsis}}}|helion}} | 2.94 astronomical unit|AU (439.95 Gm) |
|{{{apsis}}}|helion}} | 2.57 AU (384.67 Gm) |
2.76 AU (412.31 Gm) | |
Eccentricity | 0.067041 |
Orbital period | 4.58 yr (1,671.3 d) |
Average Orbital speed | 17.92 km/s |
Mean anomaly | 67.782° |
Mean motion | 0° 12m 55.44s / day |
Inclination | 8.2449° |
Longitude of ascending node | 31.154° |
94.611° | |
Earth MOID | 1.60 AU (239.57 Gm) |
Jupiter MOID | 2.11 AU (315.95 Gm) |
TJupiter | 3.325 |
Physical characteristics | |
Dimensions | 122[2] 116.14±3.93 km[3] |
Mass | (3.08 ± 1.35) × 1018 kg[3] |
Mean density | 3.75±1.68 g/cm3[3] |
Rotation period | 12.7988 h (0.53328 d)[2][4] |
Geometric albedo | 0.0557±0.0039[5] |
Physics | ~168 K |
CX[6] (Tholen) Ch[6] (Bus) | |
Absolute magnitude (H) | 8.6,[2] 8.30[5] |
Johanna (minor planet designation: 127 Johanna) is a large, dark main-belt asteroid that was discovered by French astronomers Paul Henry and Prosper Henry on 5 November 1872, and is believed to be named after Joan of Arc.[7] It is classified as a CX-type asteroid, indicating the spectrum shows properties of both a carbonaceous C-type asteroid and a metallic X-type asteroid.[6]
A photoelectric study was performed of this minor planet in 1991 at the Konkoly Observatory in Hungary. The resulting light curve showed a synodic rotation period of 6.94 ± 0.29 hours with a brightness variation of 0.2 in magnitude. It was estimated to have an absolute magnitude of 8.459 ± 0.013 with a diameter of 96–118 km (60–73 mi) and an albedo of 0.06–0.04.[8]
Infrared observations made in 1982 at Konkoly showed a rapid variation that seemed to suggest a shorter rotation period of 1.5 hours; one of the fastest known at the time. However, an irregular shape was suggested as an alternative cause of the rapid variation.[9] The present day established rotation period of this object is 12.7988 hours.[4]
During 2001, 127 Johanna was observed by radar from the Arecibo Observatory. The return signal matched an effective diameter of 117 ± 21 km.[6] A larger diameter value of 123.41 ± 4.07 km was obtained from the Midcourse Space Experiment observations, with an albedo of 0.0557 ± 0.0039.[5] A 2012 study gave a refined diameter estimate of 116.14 ± 3.93 km.[3]
References
- ↑ Noah Webster (1884) A Practical Dictionary of the English Language
- ↑ 2.0 2.1 2.2 2.3 Yeomans, Donald K., "127 Johanna", JPL Small-Body Database Browser (NASA Jet Propulsion Laboratory), https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=127, retrieved 12 May 2016.
- ↑ 3.0 3.1 3.2 3.3 Carry, B. (December 2012), "Density of asteroids", Planetary and Space Science 73: pp. 98–118, doi:10.1016/j.pss.2012.03.009, Bibcode: 2012P&SS...73...98C. See Table 1.
- ↑ 4.0 4.1 Behrend, Raoul (in French), Courbes de rotation d'astéroïdes et de comètes, Observatoire de Genève, http://obswww.unige.ch/~behrend/page_cou.html, retrieved 2013-03-29
- ↑ 5.0 5.1 5.2 Tedesco, Edward F. et al. (July 2002), "The Midcourse Space Experiment Infrared Minor Planet Survey", The Astronomical Journal 124 (124): pp. 583–591, doi:10.1086/340960, Bibcode: 2002AJ....124..583T.
- ↑ 6.0 6.1 6.2 6.3 Magri, Christopher et al. (January 2007), "A radar survey of main-belt asteroids: Arecibo observations of 55 objects during 1999–2003", Icarus 186 (1): 126–151, doi:10.1016/j.icarus.2006.08.018, Bibcode: 2007Icar..186..126M
- ↑ Schmadel, Lutz D.; International Astronomical Union (2003), Dictionary of minor planet names, Berlin; New York: Springer-Verlag, p. 27, ISBN 978-3-540-00238-3, https://books.google.com/books?id=KWrB1jPCa8AC&pg=PA27.
- ↑ Toth, Imre (December 1997), "First lightcurve observations and rotation of minor planet 127 Johanna", Planetary and Space Science 45: pp. 1625–1637, doi:10.1016/S0032-0633(97)00141-4, Bibcode: 1997P&SS...45.1625T.
- ↑ Szecsenyi-Nagy, G. (1983), "127 Johanna - Is it really the most quickly spinning asteroid known at this moment?", Asteroids, comets, meteors; Proceedings of the Meeting, Uppsala, Sweden, June 20–22, 1983 45: pp. 49–53, doi:10.1016/S0032-0633(97)00141-4, Bibcode: 1983acm..proc...49S.
External links
- 127 Johanna at AstDyS-2, Asteroids—Dynamic Site
- 127 Johanna at the JPL Small-Body Database
![]() | Original source: https://en.wikipedia.org/wiki/127 Johanna.
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