Jump to content

C/2021 O3 (PanSTARRS): Difference between revisions

Edit links
From Wikipedia, the free encyclopedia
Browse history interactively
← Previous editNext edit →
Content deleted Content added
VisualWikitext
Comment on its future evolution.
m Reference updated
Line 100: Line 100:
|last16 = Paganini-Martins |first16 = C.
|last16 = Paganini-Martins |first16 = C.
|display-authors=6
|display-authors=6
|date = 14 July 2023
|date = 20 July 2023
|title = Borderline hyperbolic comet C/2021 O3 (PANSTARRS) was fading as it approached the Sun
|title = Borderline hyperbolic comet C/2021 O3 (PANSTARRS) was fading as it approached the Sun
|journal = [[Monthly Notices of the Royal Astronomical Society]]
|journal = [[Monthly Notices of the Royal Astronomical Society]]
|volume = |number = |pages =
|volume = 524 |number = 2 |pages = 2733-2740
|s2cid = |arxiv = |doi = 10.1093/mnras/stad2111
|s2cid = |arxiv = 2307.10029 |doi = 10.1093/mnras/stad2111
|bibcode =
|bibcode = 2023MNRAS.524.2733E
|url = https://academic.oup.com/mnras/advance-article-abstract/doi/10.1093/mnras/stad2111/7224605
|url = https://academic.oup.com/mnras/article-abstract/524/2/2733/7224605
}}
}}
</ref>
</ref>


}} <!-- end of reflist -->
}} <!-- end of reflist -->

Revision as of 17:52, 23 July 2023

C/2021 O3 (PanSTARRS)
Discovery
Discovered byPan-STARRS
Discovery date26 July 2021
Orbital characteristics
Epoch2021-Aug-21
Observation arc53 days
Number of
observations		279
Orbit typeOort cloud[2]
Perihelion0.287 AU[1]
Eccentricity1.00005 (epoch 1950)[2]
1.002 (epoch 2021)[1]
1.0001 (epoch 2100)[2]
Inclination56.75°
189.03°
Argument of
periapsis		299.97°
Last perihelion21 April 2022
TJupiter0.446
Earth MOID0.062 AU[1]
Jupiter MOID2.16 AU
Comet total
magnitude (M1)		10.6

C/2021 O3 (PanSTARRS) is perhaps an Oort cloud comet, discovered on 26 July 2021 by the Pan-STARRS sky survey. It came to perihelion on 21 April 2022 at 0.287 AU (42.9 million km). from the Sun.

The comet was expected to reach apparent magnitude 5 by late April 2022, while being only 15 degrees from the Sun.[3][4] While near perihelion the comet was dimmer than expectations. It was faintly visible in STEREO/SECCHI COR2-A on 27 April 2022.[5] Observations by Lowell Discovery Telescope on April 29 in the twilight detected a diffuse glow with a magnitude of 9 where the comet was expected to be, indicating that the comet nucleus disintegrated during perihelion.[6] C/2021 O3 made its closest approach to Earth on 8 May 2022 at a distance of 0.60 AU (90 million km).[7] As a dynamically new comet from the Oort cloud there was a high risk of disintegration.[8]

The comet was recovered by multiple observatories after perihelion at magnitudes not too different from those observed pre-perihelion.[9] Calculations carried out using the pre- and post-perihelion orbits indicate that although the comet is probably dynamically old, it may also be a fragment of a dynamically new comet that was released during the first perihelion passage of its parent comet.[9]

Orbit

Orbit through inner Solar System

With a short observation arc of 7 days, the Minor Planet Center used an assumed eccentricity of 1.0 for the orbit solution.[10] Due to statistics of small numbers, with a short 10 day arc JPL had an eccentricity of 0.99595±0.00444 which could be as high as 1.00039 or as low as 0.99151.[11] With an observation arc of 53 days, JPL Horizons shows both an inbound and outbound eccentricity greater than 1.[2]

C/2021 O3 probably took millions of years to arrive from the outer Oort cloud and, had it survived, may have been fated to be ejected from the Solar System.[2] This is also the most likely scenario when considering the post-perihelion orbit determination of the surviving object.[9]

References

  1. ^ a b c "JPL Small-Body Database Browser: C/2021 O3 (PANSTARRS)". Jet Propulsion Laboratory. Retrieved 28 September 2021.
  2. ^ a b c d e "JPL Horizons On-Line Ephemeris for 2021 O3 at epoch 1950 and 2100 (barycentric)". JPL Horizons On-Line Ephemeris System. Jet Propulsion Laboratory. Retrieved 29 September 2021. Solution using the Solar System Barycenter. Ephemeris Type:Elements and Center:@0 (To be outside planetary region, inbound epoch 1950 and outbound epoch 2100. Aphelia/orbital periods defined while in the planetary-region are misleading for knowing the long-term inbound/outbound solutions.)
  3. ^ "Electronic Telegram No. 5009". Central Bureau Electronic Telegrams. 1 August 2021.
  4. ^ "C/2021 O3 ( PanSTARRS )". Seiichi Yoshida.
  5. ^ C/2021 O3 (PANSTARRS) was faintly visible
  6. ^ Zhang, Qicheng; Ye, Quanzhi; Farnham, Tony L.; Holt, Carrie E. (2 May 2022). "ATel #15358: Disintegration of Near-Sun Comet C/2021 O3 (PANSTARRS)". The Astronomer's Telegram. Retrieved 8 May 2022.
  7. ^ "Closest Approach to Earth 2022" (Closest Earth approach occurs when deldot flips from negative to positive). JPL Horizons. Retrieved 2021-09-29.
  8. ^ Machholz, Donald (5 May 2022). "EarthSky | Darn! Comet C/2021 O3 PanSTARRS has disintegrated". earthsky.org.
  9. ^ a b c Evangelista-Santana, M.; De Prá, M.; Carvano, J. M.; de la Fuente Marcos, C.; de la Fuente Marcos, R.; Alarcon, M. R.; et al. (20 July 2023). "Borderline hyperbolic comet C/2021 O3 (PANSTARRS) was fading as it approached the Sun". Monthly Notices of the Royal Astronomical Society. 524 (2): 2733–2740. arXiv:2307.10029. Bibcode:2023MNRAS.524.2733E. doi:10.1093/mnras/stad2111.{{cite journal}}: CS1 maint: unflagged free DOI (link)
  10. ^ "MPEC 2021-P05 : COMET C/2021 O3 (PANSTARRS)] (7-day arc)". Minor Planet Electronic Circulars. Minor Planet Center. 1 August 2021.
  11. ^ Archive of JPL #2 (with a 10 day arc)
Stub icon

This comet-related article is a stub. You can help Wikipedia by expanding it.

Retrieved from "https://en.wikipedia.org/w/index.php?title=C/2021_O3_(PanSTARRS)&oldid=1166776458"