C/2020 F8 (SWAN)

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C/2020 F8
Comet C/2020 F8 (SWAN) on May 1, 2020 from Indonesia
Discovery
Discovered bySolar and Heliospheric Observatory (SOHO)
Discovery dateMarch 25, 2020[1]
Designations
SWAN01[citation needed]
Orbital characteristics
Epoch2020-Apr-26
(JD 2458965.5)
Observation arc42 days
Orbit typeOort cloud
Aphelion~1300 AU (outbound)
Perihelion0.4303 AU (64 million km)
Eccentricity0.99994
Orbital periodHyperbolic trajectory (inbound)
~17000 years (outbound)
Inclination110.8
Last perihelionMay 27, 2020
Earth MOID0.1937 AU (29 million km; 75 LD)
Jupiter MOID2.35 AU

C/2020 F8 (SWAN), or Comet SWAN, is an Oort cloud comet that was discovered in images taken by the Solar Wind Anisotropies (SWAN) camera on March 25, 2020, aboard the Solar Heliospheric Observer (SOHO) spacecraft.[2][1] In the glare of twilight, Comet SWAN is difficult to find with 50mm binoculars even though it is still near the theoretical range of naked eye visibility. The comet has dimmed since May 3.[3] As of perihelion, the comet is very diffuse, does not have a visible nucleus and is not a comet that will be noticed by inexperienced observers. It is likely that the comet disintegrated.

Observing[edit]

On April 28, 2020 it had an apparent magnitude of 7 and was too diffuse to be visible to the naked eye even from a dark site.[3] The comet was also hidden by the glare of twilight, zodiacal light and atmospheric extinction. It was originally best seen from the Southern Hemisphere. It was expected to possibly reach 3rd magnitude in May, but instead hovered closer to magnitude 6.[4] In either case it was near the glare of twilight, which made it appear significantly fainter.[4] On May 2, the comet had reached a magnitude of 4.7 and had been detected with naked eye,[5] the tail had a visual length of one degree and could be traced photographically for 6-8 degrees.[6] After that the comet faded, probably as the nucleus of the comet fragmented.[7][8] It passed through the celestial equator on 7 May, then it headed northward and it was near the 2nd magnitude star Algol on 20 May.[1] It passed its perihelion on May 27, 2020.

Sky trajectory with 7 week markers

Orbit[edit]

C/2020 F8 (SWAN)'s orbit

The Minor Planet Center initially listed the orbit as bound with .[2] With a short 18-day observation arc JPL listed the comet as hyperbolic with an eccentricity of 1.0009±0.001, but a longer observation arc was needed to refine the uncertainties and either confirm its hyperbolic trajectory, or determine its orbital period of thousands or millions of years.[9] With a 40-day observation arc it was possible to determine that it came from the Oort cloud on a Hyperbolic trajectory and that the outbound orbit will last ~11,000 years.

On May 12, 2020, the comet passed about 0.56 AU (84 million km; 220 LD) from Earth. On May 27, 2020 the comet came to perihelion 0.43 AU (64 million km) from the Sun.[2]

Gallery[edit]

References[edit]

  1. ^ a b c "Comet Y4 ATLAS Breaks Up...Enter Comet F8 SWAN". Universe Today. April 15, 2020. Retrieved April 16, 2020.
  2. ^ a b c "MPEC 2020-G94 : COMET C/2020 F8 (SWAN)". minorplanetcenter.net. Retrieved April 16, 2020.
  3. ^ a b Ghosh, Trinankur. "Comet Observation database (COBS)". Retrieved April 28, 2020. "C/2020 F8 (SWAN) plot" Archived June 10, 2020, at the Wayback Machine
  4. ^ a b Seiichi Yoshida (April 13, 2020). "C/2020 F8 ( SWAN )". Retrieved April 16, 2020.
  5. ^ "Comet C/2020 F8 (SWAN) observation list". cobs.si. Retrieved January 22, 2023.
  6. ^ King, Bob (May 6, 2020). "Comet SWAN Expected to Put on a Splendid Show". Sky & Telescope. Retrieved January 6, 2022.
  7. ^ Joe Rao (May 12, 2020). "Newfound Comet SWAN could soon fizzle out of view". Space.com. Retrieved January 22, 2023.
  8. ^ King, Bob (May 22, 2020). "Comet SWAN's Final Song". Sky & Telescope. Retrieved January 22, 2023.
  9. ^ "JPL Small-Body Database Browser: C/2020 F8 (SWAN)". Jet Propulsion Laboratory. Archived from the original on April 17, 2020. Retrieved April 30, 2020.
  10. ^ Diego Toscan. "Comet C/2020 F8 SWAN 2 May 2020". Archived from the original on December 24, 2021. Retrieved May 4, 2020.

External links[edit]