Английская Википедия:C/2020 F8 (SWAN)

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Шаблон:Short description Шаблон:Use mdy dates Шаблон:Infobox comet

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.[1][2] 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

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.[2] It passed its perihelion on May 27, 2020.

Файл:C2020 F8-skypath.png
Sky trajectory with 7 week markers

Orbit

Файл:C 2020 F8 SWAN.jpg
C/2020 F8 (SWAN)'s orbit

The Minor Planet Center initially listed the orbit as bound with <math>e<1</math>.[1] With a short 18-day observation arc JPL listed the comet as hyperbolic with an eccentricity of Шаблон:Val, 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 Шаблон:Convert from Earth. On May 27, 2020 the comet came to perihelion Шаблон:Convert from the Sun.[1]

Gallery

References

Шаблон:Reflist

External links


Шаблон:Comet-stub

Шаблон:2020 in space Шаблон:Comets Шаблон:Authority control

  1. 1,0 1,1 1,2 Шаблон:Cite web
  2. 2,0 2,1 Шаблон:Cite web
  3. 3,0 3,1 Ошибка цитирования Неверный тег <ref>; для сносок COBS не указан текст
  4. 4,0 4,1 Ошибка цитирования Неверный тег <ref>; для сносок Yoshida не указан текст
  5. Шаблон:Cite web
  6. Шаблон:Cite web
  7. Шаблон:Cite journal
  8. Шаблон:Cite web
  9. Ошибка цитирования Неверный тег <ref>; для сносок jpldata не указан текст
  10. Ошибка цитирования Неверный тег <ref>; для сносок photo не указан текст