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{{For|the other comet discovered by Ferdinand Quénisset|C/1893 N1 (Rordame–Quénisset)}} | {{For|the other comet discovered by Ferdinand Quénisset|C/1893 N1 (Rordame–Quénisset)}} | ||
{{Infobox comet | {{Infobox comet | ||
| name = C/1911 S2 (Quénisset) | |||
| image = C1911 S2 (Quenisset) on 24 September 1911.jpg | | image = C1911 S2 (Quenisset) on 24 September 1911.jpg | ||
| caption = Comet Quénisset photographed from ] on 24 September 1911 | | caption = Comet Quénisset photographed from ] on 24 September 1911 | ||
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| discoverer = ] | | discoverer = ] | ||
| discovery_site = ], France | | discovery_site = ], France | ||
| discovery_date = 23 September 1911 | |||
| designations = 1911f{{r|ICQ1}}<br>1911 VI | | designations = 1911f{{r|ICQ1}}<br>1911 VI | ||
| orbit_ref = {{r|jpl}} | | orbit_ref = {{r|jpl}} | ||
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}} | }} | ||
'''Comet Quénisset''', also known by its modern formal designation '''C/1911 S2''', is a ] that has a 4,000-year retrograde orbit around the ]. It is the second of two |
'''Comet Quénisset''', also known by its modern formal designation '''C/1911 S2''', is a ] that has a 4,000-year retrograde orbit around the ]. It is the second of two ]s discovered by French astronomer, ].{{r|Baldet_1911}} | ||
== Potential meteor shower == | |||
Orbital calculations by J. B. Dale revealed that although there would be no close encounter between the comet and the ], the former's descending node resulted in a ] of about {{convert|0.0172|AU|e6km|abbr=unit}} by 16 December 1911.{{r|Dale_1911}} This has led to other scientists predicting a ] originating from this comet that will be coming from the constellation ] on April 27 of each year, though none has been observed so far.{{r|Davidson_1920}} | |||
== References == | == References == | ||
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| bibcode= 1911LAstr..25..436B | | bibcode= 1911LAstr..25..436B | ||
| language= fr }} | | language= fr }} | ||
</ref> | |||
<ref name="Dale_1911">{{cite journal | |||
| author1= J. B. Dale | |||
| title= Elements of Comet 1911f | |||
| url= https://www.nature.com/articles/087450b0.pdf | |||
| journal= Nature | |||
| year= 1911 | |||
| volume= 87 | |||
| issue= 2188 | |||
| page= 450 | |||
| doi= 10.1038/087450b0 | |||
| doi-access= free }} | |||
</ref> | |||
<ref name="Davidson_1920">{{cite journal | |||
| author1= M. Davidson | |||
| title= Council Cometary radiant points, 1875-1920 | |||
| url= https://academic.oup.com/mnras/article-pdf/80/8/739/3654970/mnras80-0739.pdf | |||
| journal= Monthly Notices of the Royal Astronomical Society | |||
| year= 1920 | |||
| volume= 80 | |||
| issue= 8 | |||
| pages= 739–741 | |||
| bibcode= 1920MNRAS..80..739D | |||
| doi= 10.1093/mnras/80.8.739 | |||
| doi-access= free }} | |||
</ref> | </ref> | ||
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{{DEFAULTSORT:Quénisset, 1911 S2}} | {{DEFAULTSORT:Quénisset, 1911 S2}} | ||
] | ] | ||
] | |||
{{Comet-stub}} | {{Comet-stub}} |
Latest revision as of 06:11, 20 December 2024
Non-periodic comet For the other comet discovered by Ferdinand Quénisset, see C/1893 N1 (Rordame–Quénisset).Comet Quénisset photographed from Juvisy-sur-Orge, France on 24 September 1911 | |
Discovery | |
---|---|
Discovered by | Ferdinand Quénisset |
Discovery site | Flammarion Obs, France |
Discovery date | 23 September 1911 |
Designations | |
Alternative designations | 1911f 1911 VI |
Orbital characteristics | |
Epoch | 25 October 1911 (JD 2419334.5) |
Observation arc | 30 days |
Number of observations | 9 |
Aphelion | 517.6 AU |
Perihelion | 0.787 AU |
Semi-major axis | 259.2 AU |
Eccentricity | 0.78735 |
Orbital period | ~4,170 years |
Inclination | 108.09° |
Longitude of ascending node | 36.430° |
Argument of periapsis | 122.09° |
Last perihelion | 12 November 1911 |
Earth MOID | 0.0172 AU |
Jupiter MOID | 0.7418 AU |
Comet Quénisset, also known by its modern formal designation C/1911 S2, is a non-periodic comet that has a 4,000-year retrograde orbit around the Sun. It is the second of two comets discovered by French astronomer, Ferdinand Quénisset.
Potential meteor shower
Orbital calculations by J. B. Dale revealed that although there would be no close encounter between the comet and the Earth, the former's descending node resulted in a minimum orbit intersection distance of about 0.0172 AU (2.57 million km) by 16 December 1911. This has led to other scientists predicting a meteor shower originating from this comet that will be coming from the constellation Vulpecula on April 27 of each year, though none has been observed so far.
References
- ^ M. M. Baldet; F. Quénisset (1911). "Découverte d'une Comète a l'Observatoire Flammarion de Juvisy" [Discovery of a Comet at the Flammarion Observatory in Juvisy]. L'Astronomie (in French). 25 (1): 436–437. Bibcode:1911LAstr..25..436B.
- "Comet Names and Designations". International Comet Quarterly. Retrieved 20 December 2024.
- "C/1911 S2 (Quénisset) – JPL Small-Body Database Lookup". ssd.jpl.nasa.gov. Jet Propulsion Laboratory. Retrieved 28 March 2024.
- J. B. Dale (1911). "Elements of Comet 1911f" (PDF). Nature. 87 (2188): 450. doi:10.1038/087450b0.
- M. Davidson (1920). "Council Cometary radiant points, 1875-1920" (PDF). Monthly Notices of the Royal Astronomical Society. 80 (8): 739–741. Bibcode:1920MNRAS..80..739D. doi:10.1093/mnras/80.8.739.
External links
- C/1911 S2 at the JPL Small-Body Database
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