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127 Johanna
Reference material by Wikipedia contributors. This retains its source identity and is not 411 news reporting.
Main-belt asteroid
September 2018
yes #D6D6D6 127 Johanna 127Johanna (Lightcurve Inversion).png A three-dimensional model of 127 Johanna based on its lightcurve Paul Henry and Prosper Henry 5 November 1872 (127) Johanna A872 VB dʒ oʊ- ' h æ n əNoah Webster (1884) A Practical Dictionary of the English Language Joan of Arc Main belt 31 July 2016 (JD 2457600.5) 2.75615 AU Gm ri2 2 on 2.57138 AU Gm ri2 2 on 2.9409 AU Gm ri2 2 on on 0.067041 1671.3 days years 2 flip on 8.2449° 31.154° 94.611° 67.782° 17.92 km/s 122116.14 3.93 km (3.08 ± 1.35) × 1018 kg 3.75 1.68 g/cm3 12.7988 h d on on CX (Tholen)Ch (Bus) 8.6, 8.30 0.0557 0.0039 ~168 K 0.21540 ms / day 98.53 yr (35989 d) 0 1.60141 AU Gm ri2 2 on 2.11199 AU Gm ri2 2 on 3.325
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. 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.
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 and an albedo of 0.06–0.04.
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. The present day established rotation period of this object is 12.7988 hours.
During 2001, 127 Johanna was observed by radar from the Arecibo Observatory. The return signal matched an effective diameter of 117 ± 21 km. 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. A 2012 study gave a refined diameter estimate of 116.14 ± 3.93 km.
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2013-03-29
29 July 2016
https://web.archive.org/web/20160729213840/http://obswww.unige.ch/~behrend/page_cou.html
dead
External links
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126 Velleda 127 128 Nemesis
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Category:Discoveries by Paul Henry and Prosper Henry
Category:Named minor planets
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