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C/2014 E2 (Jacques)

From Wikipedia, the free encyclopedia
Long-period comet
C/2014 E2 (Jacques)
Image of 2014 E2 (Jacques) in 24 August 2014
Discovery
Discovered byCristóvão Jacques
Eduardo Pimentel
João Ribeiro de Barros
Marcelo Dias
Discovery date13 March 2014
Orbital characteristics[2]
Epoch2014 May 23.0 TT
(JD 2456800.5)
Aphelion~1600AU (epoch 1950)[1]
Perihelion0.6638 AU (q)
Eccentricity0.99912 (e)
Orbital period~22,000 years inbound (Barycentric solution forepoch 1950)[1]
~12,000 years outbound
(Barycentric solution forepoch 2050)[1]
Avg.orbital speed27 km/s
Max.orbital speed51.7 km/s
Inclination156.4° (i)
Last perihelion2014 July 2

C/2014 E2 (Jacques), provisionally designated as S002692,[3] is a long-periodcomet discovered by the Brazilian astronomers Cristóvão Jacques Lage de Faria, Eduardo Pimentel, João Ribeiro de Barros and Marcelo Dias on the night of 13 March 2014.[4] It was the second comet discovered by the SONEAR Observatory team after comet C/2014 A4.

Overview

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Observations were made with a 0.45-meter (17.7-inch)f/2.9 wide-fieldreflector telescope withequatorial assembly andCCD camera at the Southern Observatory for Near Earth Asteroids Research (SONEAR), located near Oliveira, Minas Gerais, Brazil.[5]

In late March 2014, C/2014 E2 (Jacques) appeared to contain a dense, brightcoma (11.5-12magnitude), visible with an 8-inch telescope.[5] It crossed thecelestial equator on 8 May 2014 becoming aNorthern Hemisphere object.[6] From 3 June 2014 until 17 July 2014 it had anelongation less than 30 degrees from the Sun.[6] The comet was visible inLASCO C3 on 21 June 2014.[7] C/2014 E2 peaked around apparent magnitude 6 in mid-July and was visible in binoculars above the glow of morningtwilight.[8][9]

C/2014 E2 passed 0.085 AU (12,700,000 km; 7,900,000 mi) from Venus on 13 July 2014.[10] On 20 July 2014 the comet was near the naked eye starBeta Tauri.[11] On 22 August 2014 it passedEpsilon Cassiopeiae. It reachedperigee (closest approach to Earth) on 28 August 2014, at 0.56 AU (84,000,000 km; 52,000,000 mi).[3] The comet passed about 3 degrees fromDeneb from 4–5 September 2014.[12] On 14 September the comet was nearAlbireo.[13]

By October 2014 the comet had fainted to magnitude 10.[14]

References

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  1. ^abcHorizons output."Barycentric Osculating Orbital Elements for Comet C/2014 E2 (Jacques)". (Solution using the Solar SystemBarycenter andbarycentric coordinates. Select Ephemeris Type:Elements and Center:@0)
  2. ^"C/2014 E2 (Jacques)".Small-Body Database Lookup. ssd.jpl.nasa.gov. Retrieved9 June 2024.
  3. ^ab"C/2014 E2 Jacques" (in Portuguese). Costeira1 e Cometas/REA. Retrieved2014-03-31.
  4. ^Villamarin, Jenalyn (2014-03-17)."2014 Comet Jacques: SONEAR Team in Brazil Spots New Comet C/2014 E2, Closest Approach to the Sun to Occur on June 29". International Business Times AU. Archived fromthe original on 2014-03-28. Retrieved2014-03-31.
  5. ^abKing, Bob (2014-03-15)."New Comet Jacques May Pass 8.4 million miles from Venus this July".Universe Today. Retrieved2014-03-31.
  6. ^ab"Elements and Ephemeris for C/2014 E2 (Jacques)". The International Astronomical Union Minor Planet Center. Archived fromthe original on 2014-10-26. Retrieved2014-06-15.
  7. ^Rob Kaufman – comets-ml
  8. ^Yoshida, Seiichi (2014-07-20)."Weekly Information about Bright Comets (2014 July 19: North)". aerith.net. Retrieved2014-10-21.
  9. ^Seiichi Yoshida."C/2014 E2 ( Jacques )". Seiichi Yoshida's Comet Catalog. Retrieved2014-06-15.
  10. ^"JPL Close-Approach Data: C/2014 E2 (Jacques)" (last observation: 2014-10-05;arc: 206 days). Retrieved2014-04-30.
  11. ^"Catch Comet Jacques near Venus at dawn". AstroBob. 2014-07-15. Archived fromthe original on 2014-07-21. Retrieved2014-07-20.
  12. ^"Jacques S&T final Aug_Sept_edited-3". 18 August 2014.
  13. ^David Dickinson (2014-09-09)."Tales (Tails?) Of Three Comets". Universe Today. Retrieved2014-09-12.
  14. ^Yoshida, Seiichi (2014-10-05)."Weekly Information about Bright Comets (2014 Oct. 4: North)". aerith.net. Retrieved2014-10-21.

External links

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Wikimedia Commons has media related toC/2014 E2.
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