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C/2012 K1 (PanSTARRS)

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Oort cloud comet
Not to be confused with the cometC/2011 L4 (PanSTARRS) that became bright in March 2013.

C/2012 K1 (PanSTARRS)
NEOWISE series ofinfrared images of C/2012 K1 on 20 May 2014
Discovery
Discovered byPan-STARRS
1.8-mRitchey–Chrétien (F51)[1]
Discovery date17 May 2012
Orbital characteristics
Epoch11 August 2014[2]
Orbit typeOort cloud
Aphelion~52000AU (inbound)[3]
~14000 AU (outbound)
Perihelion1.0545AU (q)[2]
Eccentricity1.00021[2]
Orbital periodseveral million years inbound (Barycentric solution forepoch 1950)[3]
~600000yr outbound
(Barycentric solution for epoch 2050)[3]
Inclination142.43°[2]
Last perihelion27 August 2014[2]
JupiterMOID1.5 AU
Physical characteristics[4][5]
Dimensions2.4–4.4 km (1.5–2.7 mi)
Mean diameter
3.4 km (2.1 mi)
9.4±0.4 hours

C/2012 K1 (PanSTARRS) is aretrogradeOort cloudcomet discovered at magnitude 19.7, 8.7AU from the Sun on 17 May 2012 using thePan-STARRS telescope located near the summit ofHaleakalā, on the island ofMaui inHawaii (U.S.).[1]

The comet started 2014 as a Northern Hemisphere object. By late April 2014 it had brightened to roughlyapparent magnitude ~8.8[6] making it a small telescope/binoculars target for experienced observers. In June and July 2014 the comet was near theSickle of Leo.[7] As of 3 July 2014 the comet had brightened to magnitude 7.9.[8]

From 12 July 2014 until 6 September 2014 it had anelongation less than 30 degrees from the Sun.[6] The comet came toperihelion (closest approach to the Sun) on 27 August 2014 at a distance of 1.05 AU (157,000,000 km; 98,000,000 mi) from the Sun.[2] It crosses thecelestial equator on 15 September 2014 becoming a Southern Hemisphere object.[6]

The comet peaked around magnitude 6.9 in mid-October 2014[9][10] when it had anelongation of around 75 degrees from the Sun.[6] It is visible in binoculars and small telescopes.

References

[edit]
  1. ^ab"MPEC 2012-K36 : COMET C/2012 K1 (PANSTARRS)".IAU Minor Planet Center. 21 May 2012. Retrieved5 May 2013. (CK12K010)
  2. ^abcdef"MPEC 2014-K54: Observations and Orbits of Comets". IAU Minor Planet Center. 26 May 2014. Retrieved15 June 2014.
  3. ^abcHorizons output."Barycentric Osculating Orbital Elements for Comet C/2012 K1 (PANSTARRS)". Solution using the Solar SystemBarycenter. Ephemeris Type:Elements and Center:@0 (To be outside planetary region, inbound epoch 1950 and outbound epoch 2050)
  4. ^D. C. Jewitt (2022)."Destruction of Long-period Comets".Astronomical Journal.164 (4):158–166.arXiv:2208.04469.Bibcode:2022AJ....164..158J.doi:10.3847/1538-3881/ac886d.
  5. ^M. M. Knight; R. Kokotanekova; N. H. Samarasinha (2023). "Physical and Surface Properties of Comet Nuclei from Remote Observations".arXiv:2304.09309 [astro-ph.EP].
  6. ^abcd"Elements and Ephemeris for C/2012 K1 (PANSTARRS)". IAU Minor Planet Center. Archived fromthe original on 28 August 2013. Retrieved5 May 2013.
  7. ^Bob King (11 June 2014)."Comet PanSTARRS Keeps Getting Better".Sky & Telescope.
  8. ^Seiichi Yoshida (20 July 2014)."Weekly Information about Bright Comets (2014 July 5: North)". Seiichi Yoshida's Comet Catalog. Retrieved23 July 2014.[permanent dead link]
  9. ^Yoshida, Seiichi (20 October 2014)."Weekly Information about Bright Comets (2014 Oct. 18: South)". aerith.net. Retrieved21 October 2014.
  10. ^Seiichi Yoshida (29 April 2013)."C/2012 K1 ( PanSTARRS )". Seiichi Yoshida's Comet Catalog. Retrieved5 May 2013.

External links

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