Ryves Comet
Comet
| Discovery | |
|---|---|
| Discovered by | Percy Mayow Ryves |
| Discovery date | August 10, 1931 |
| Designations | |
| 1931c; 1931 E; C/1931 P1 | |
| Orbital characteristics[1] | |
| Epoch | 7 August 1931 |
| Aphelion | 222 AU |
| Perihelion | 0.075 AU |
| Semi-major axis | 111 AU |
| Eccentricity | 0.999326 |
| Orbital period | N/A |
| Inclination | 169.29° |
Longitude of ascending node | 102.28° |
| Argument of periapsis | 168.15° |
| Last perihelion | 25 August 1931 |
Ryves Comet, also known as C/1931 P1, 1931 E or 1931c, was discovered by Percy Mayow Ryves, an English amateur astronomer, on August 10, 1931. The comet passed perihelion on 25 August 1931 at a distance of 7 million miles from the Sun.[2]
Observational history
The comet was discovered by amateur astronomer Percy Mayow Ryves on 10 August 1931.[3] His find was made using a small telescope in Zaragoza, Spain.[citation needed] He noted that the comet was faintly visible with naked eye.[3] The comet was later observed from the Yerkes Observatory and the University of California Leuschner Observatory. George van Biesbroeck observed the comet on 14 August 1931 and noted it had a tail one degree long and estimated its apparent magnitude to be 4.[4]
It appeared as a ball of hot gas traveling at one hundred miles per second from the Naval Observatory. Soon the comet became unobservable as it passed between the Sun and Earth.[3] The comet passed within 7,000,000 miles of the Sun[2] on August 25. It is estimated that became as bright as Venus, however it was too close to the Sun and the horizon to be observed. It then moved towards the far side of the Sun.[3]
Ryves Comet was recovered in early October and its brightness was estimated to be of ninth magnitude by October 9, 1931, and was not observable with the naked eye. Astronomers at the Yerkes Observatory waited until just prior to dawn to observe and photograph it. The comet came into view just ahead of the Sun. Yerkes Observatory director, Edwin B. Frost, determined that Ryves Comet was two hours east of the Sun and seven degrees removed from it. In October it was one hundred times fainter than when it was first observed in August.[5] Its coma had then an estimated diameter of 3−4 arcminutes and its tail was estimated photographically to be three quarters of a degree long and facing towards the Sun.[6]
Its orbit indicates that it approached Jupiter down to 0.15 astronomical units (22×10^6 km; 14×10^6 mi) resulting to a hyperbolic orbit before perihelion.[7]
References
- ^ "Small-Body Database Lookup: C/1931 P1 (Ryves)". ssd.jpl.nasa.gov. Retrieved 22 January 2024.
- ^ a b "Ryves Comet Passes at 100 Miles a Second; Heads for Void, Probably Never to Return". New York Times. August 28, 1931. p. 13.
- ^ a b c d Bower, E. C.; Miller, Mary L. (October 1931). "Comet 1931c (Ryves)". Publications of the Astronomical Society of the Pacific. 43 (255): 357. Bibcode:1931PASP...43..357B. doi:10.1086/124164.
- ^ Ryves, P. M.; Shapley, H.; van Biesbroeck, G. (15 August 1931). "Comet Ryves (1931c)". International Astronomical Union Circular (331): 1. ISSN 0081-0304.
- ^ "Elusive Ryves Comet Is Photographed; Yerkes Observer Gets Picture as Wanderer Rises on Horizon Ahead of Sun". New York Times. October 9, 1931. p. 2.
- ^ van Biesbroeck, G. (1931). "Comet Notes: Comet 1931 c (Ryves)". Popular Astronomy. 39: 546. Bibcode:1931PA.....39..546V. ISSN 0197-7482.
- ^ Bower, Ernest Clare; Miller, Mary L. (1931). "Elements and ephemeris of Comet 1931c (Ryves)". Lick Observatory Bulletins. 15: 179–180. Bibcode:1931LicOB..15..179B. doi:10.5479/ADS/bib/1931LicOB.15.179B.
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