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Revision as of 10:37, 30 December 2024 editKyloRen2017 (talk | contribs)Extended confirmed users5,127 editsmNo edit summary← Previous edit Revision as of 11:25, 30 December 2024 edit undoKyloRen2017 (talk | contribs)Extended confirmed users5,127 edits Orbit: Relationship with comets Liller (1988 A1), SWAN (2015 F3) and Leonard (2023 V5)Next edit →
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'''C/1996 Q1 (Tabur)''' is a ] that was expected to appear in the naked eye in but faded rapidly before doing so in 1996.{{r|cometography}} It is the first of three comets discovered by Australian astronomer, ]. '''C/1996 Q1 (Tabur)''' is a ] that was expected to appear in the naked eye in but faded rapidly before doing so in 1996.{{r|cometography}} It is the first of three comets discovered by Australian astronomer, ].

== Orbit ==
Shortly after discovery, ] computed the first parabolic orbit of the comet on 23 August 1996, which was roughly 73 degrees inclined to the ] and an orbital period of approximately 18,500 years.{{r|IAUC_6460}} A revised orbit was published about a week later, and ] noted it has a strong resemblance to the orbit of ], suggesting it might have fragmented from each other in a previous perihelion, despite the latter's shorter orbital period of 2,900 years.{{r|IAUC_6464}} In the following years, more fragments of the same comet family were found, ]{{r|Sekanina_2016}} and ].{{r|dela_Fuente_Marcos_2023}}


== References == == References ==
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| journal= Central Bureau for Astronomical Telegrams | journal= Central Bureau for Astronomical Telegrams
| volume= 6460 | volume= 6460
| date= 23 August 1996 }}
</ref>

<ref name="IAUC_6464">{{cite journal
| author1= B. G. Marsden
| title= Comet C/1996 Q1 (Tabur)
| url= http://www.cbat.eps.harvard.edu/iauc/06400/06464.html
| journal= Central Bureau for Astronomical Telegrams
| volume= 6464
| date= 23 August 1996 }} | date= 23 August 1996 }}
</ref> </ref>
Line 55: Line 67:
| website= ssd.jpl.nasa.gov | website= ssd.jpl.nasa.gov
| publisher= ] | publisher= ]
| access-date= 30 December 2024 }} | access-date= 21 November 2023 }}
</ref>

<ref name="Sekanina_2016">{{Cite journal
| author1= Z. Sekanina
| author2= R. Kracht
| title= Pairs and Groups of Genetically Related Long-period Comets and Proposed Identity of the Mysterious Lick Object of 1921
| url= https://arxiv.org/pdf/1510.06445
| journal= ]
| year= 2016
| volume= 823
| issue= 1
| pages= 2–28
| bibcode= 2016ApJ...823....2S
| arxiv= 1510.06445
| doi= 10.3847/0004-637X/823/1/2
| doi-access= free }}
</ref>

<ref name="dela_Fuente_Marcos_2023">{{Cite journal
| author1= C. dela Fuente Marcos
| author2= R. dela Fuente Marcos
| year= 2023
| title= Second-generation Fragments of a Comet Split in the Making: The Liller Family Comets
| url= https://iopscience.iop.org/article/10.3847/2515-5172/ad0f27/ampdf
| journal= Research Notes of the American Astronomical Society
| volume= 7
| issue= 11
| pages= 249–251
| bibcode= 2023RNAAS...7..249D
| doi= 10.3847/2515-5172/ad0f27
| doi-access= free }}
</ref> </ref>



Revision as of 11:25, 30 December 2024

Non-periodic comet For other comets discovered by Vello Tabur, see C/1997 N1 (Tabur) and C/2003 T3 (Tabur).
C/1996 Q1 (Tabur)
Discovery
Discovered byVello Tabur
Discovery siteWanniassa, Australia
Discovery date19 August 1996
Orbital characteristics
Epoch15 September 1996 (JD 2450341.5)
Observation arc58 days
Number of
observations
214
Semi-major axis605.019 AU
Eccentricity0.99861
Orbital period~14,900 years
Inclination73.356°
Longitude of
ascending node
31.400°
Argument of
periapsis
57.413°
Last perihelion3 November 1996
TJupiter0.334
Earth MOID0.0838 AU
Jupiter MOID1.0053 AU
Physical characteristics
Comet total
magnitude
(M1)
11.0
Comet nuclear
magnitude (M2)
16.4
Apparent magnitude4.8
(1996 apparition)

C/1996 Q1 (Tabur) is a non-periodic comets that was expected to appear in the naked eye in but faded rapidly before doing so in 1996. It is the first of three comets discovered by Australian astronomer, Vello Tabur.

Orbit

Shortly after discovery, Brian G. Marsden computed the first parabolic orbit of the comet on 23 August 1996, which was roughly 73 degrees inclined to the ecliptic and an orbital period of approximately 18,500 years. A revised orbit was published about a week later, and Jost Jahn noted it has a strong resemblance to the orbit of C/1988 A1 (Liller), suggesting it might have fragmented from each other in a previous perihelion, despite the latter's shorter orbital period of 2,900 years. In the following years, more fragments of the same comet family were found, C/2015 F3 (SWAN) and C/2023 V5 (Leonard).

References

  1. ^ B. G. Marsden (23 August 1996). "Comet C/1996 Q1 (Tabur)". Central Bureau for Astronomical Telegrams. 6460.
  2. "C/1996 Q1 (Tabur) – JPL Small-Body Database Lookup". ssd.jpl.nasa.gov. Jet Propulsion Laboratory. Retrieved 21 November 2023.
  3. ^ G. W. Kronk. "C/1996 Q1 (Tabur)". Cometography.com. Retrieved 30 December 2024.
  4. B. G. Marsden (23 August 1996). "Comet C/1996 Q1 (Tabur)". Central Bureau for Astronomical Telegrams. 6464.
  5. Z. Sekanina; R. Kracht (2016). "Pairs and Groups of Genetically Related Long-period Comets and Proposed Identity of the Mysterious Lick Object of 1921". The Astrophysical Journal. 823 (1): 2–28. arXiv:1510.06445. Bibcode:2016ApJ...823....2S. doi:10.3847/0004-637X/823/1/2.
  6. C. dela Fuente Marcos; R. dela Fuente Marcos (2023). "Second-generation Fragments of a Comet Split in the Making: The Liller Family Comets". Research Notes of the American Astronomical Society. 7 (11): 249–251. Bibcode:2023RNAAS...7..249D. doi:10.3847/2515-5172/ad0f27.

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