Comet Encke

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2P/Encke
Comet Encke
Discovery
Discovered by Pierre Méchain;
Johann Franz Encke (recognition of periodicity)
Discovery date 1786
Alternative
designations		 1786 I; 1795; 1805;
1819 I; 1822 II; 1825 III;
1829; 1832 I; 1835 II;
1838; 1842 I; 1845 IV
Orbital characteristics A
Epoch September 22, 2006 (JD 2454000.5)
Aphelion 4.11 AU
Perihelion 0.3302 AU
Semi-major axis 2.2178 AU
Eccentricity 0.8471
Orbital period 3.30 a
Inclination 11.76°
TJupiter 3.026[1]
Dimensions 4.8km[1]
Last perihelion 21 November 2013[1][2]
Next perihelion 10 March 2017

Comet Encke or Encke's Comet (official designation: 2P/Encke) is a periodic comet that completes an orbit of the Sun once every 3.3 years. (This is the shortest period of a reasonably bright comet; the faint main-belt comet 311P/PANSTARRS has a period of 3.2 years.) Encke was first recorded by Pierre Méchain in 1786, but it was not recognized as a periodic comet until 1819 when its orbit was computed by Johann Franz Encke; like Halley's Comet, it is unusual in being named after the calculator of its orbit rather than its discoverer. Like most comets, it has a very low albedo, reflecting only 4.6% of the light it receives. The diameter of the nucleus of Encke's Comet is 4.8 km.[1]

Discovery

As its official designation implies, Encke's Comet was the first periodic comet discovered after Halley's Comet (designated 1P/Halley). It was independently observed by several astronomers, the second being Caroline Herschel in 1795 [3] and the third Jean-Louis Pons in 1818.[4] Its orbit was calculated by Johann Franz Encke, who through laborious calculations was able to link observations of comets in 1786 (designated 2P/1786 B1), 1795 (2P/1795 V1), 1805 (2P/1805 U1) and 1818 (2P/1818 W1) to the same object. In 1819 he published his conclusions in the journal Correspondance astronomique, and predicted correctly its return in 1822 (2P/1822 L1). It was recovered by Carl Ludwig Christian Rümker at Parramatta Observatory on 2 June 1822.[5]

Orbit

Comets are in unstable orbits that evolve over time due to perturbations and outgassing. Given Encke's low orbital inclination near the ecliptic and brief orbital period of 3 years, the orbit of Encke is frequently perturbed by the inner planets.[6]

Encke's orbit gets as close as 0.17309 AU (25,894,000 km; 16,090,000 mi) to Earth (minimum orbit intersection distance).[6] On 4 July 1997, Encke passed 0.19 AU from Earth, and on June 29, 2172 it will make a close approach of roughly 0.1735 AU.[6] On 18 November 2013, it passed 0.02496 AU (3,734,000 km; 2,320,000 mi) from Mercury.[6] Close approaches to Earth usually occur every 33 years.

Observations

The failed CONTOUR mission was launched to study this comet, and also Schwassmann-Wachmann 3.

Encke's Comet loses its tail

On April 20, 2007, STEREO-A observed the tail of Comet Encke to be temporarily torn off by magnetic field disturbances caused by a coronal mass ejection (a blast of solar particles from the Sun).[7] The tail grew back due to the continuous shedding of dust and gas by the comet.[8]

Meteor showers

A Spitzer image of Encke and its debris trail in infrared light.

Comet Encke is believed to be the originator of several related meteor showers known as the Taurids (which are encountered as the Northern and Southern Taurids across November, and the Beta Taurids in late June and early July).[9][10] A shower has similarly been reported affecting Mercury.[11]

Near-Earth object 2004 TG10 may be a fragment of Encke.[12]

Mercury

Measurements on board the NASA satellite MESSENGER have revealed Encke may contribute to seasonal meteor showers on Mercury. The Mercury Atmospheric and Surface Composition Spectrometer (MASCS) instrument discovered seasonal surges of calcium since the probe began orbiting the planet in March 2011. The spikes in calcium levels are thought to originate from small dust partials hitting the planet and knocking calcium-bearing molecules into the atmosphere in a process called impact vaporization. However, the general background of interplanetary dust in the inner Solar System cannot, by itself, account for the periodic spikes in calcium. This suggests a periodic source of additional dust, for example, a cometary debris field.[13]

Effects on Earth

More than one theory has associated Encke's Comet with impacts of cometary material on Earth, and with cultural significance.

The Tunguska event of 1908, probably caused by the impact of a cometary body, has also been postulated by Czechoslovakian astronomer Ľubor Kresák as a fragment of Comet Encke.[14]

A Han Dynasty silk comet atlas, featuring drawings of comets believed by Victor Clube and Bill Napier to be related to the breakup of Encke's Comet in the past

A theory holds that the ancient symbol of the swastika appeared in a variety of cultures across the world at a similar time, and could have been inspired by the appearance of a comet from head on, as the curved jets would be reminiscent of the swastika shape (see Comets and the swastika motif). Comet Encke has sometimes been identified as the comet in question. In their 1982 book Cosmic Serpent (page 155) Victor Clube and Bill Napier reproduce an ancient Chinese catalogue of cometary shapes from the Mawangdui Silk Texts, which includes a swastika-shaped comet, and suggest that some comet drawings were related to the breakup of the progenitor of Encke and the Taurid meteoroid stream. Fred Whipple in his The Mystery of Comets (1985, page 163) points out that Comet Encke's polar axis is only 5 degrees from its orbital plane: such an orientation is ideal to have presented a pinwheel like aspect to our ancestors when Encke was more active.

Importance in the scientific history of luminiferous aether

Comet Encke (and Biela's Comet) had a role in scientific history in the generally discredited concept of luminiferous aether. As its orbit was perturbed and shortened, the shortening could only be ascribed to the drag of an "ether" through which it orbited in outer space. One reference, [1], reads:

Encke's comet is found to lose about two days in each successive period of 1200 days. Biela's comet, with twice that length of period, loses about one day. That is, the successive returns of these bodies is found to be accelerated by this amount. No other cause for this irregularity has been found but the agency of the supposed ether.

Gallery

  • A MESSENGER image of Comet Encke at its closest approach to Mercury, 17/11/2013.[15] (NASA/JHUAPL/Carnegie Institution of Washington)

  • Comet Encke as rendered in Celestia using data acquired from Earth-based observations.

  • Comet Encke with a cometary tail as rendered in Celestia using data acquired from Earth-based observations.

References

  1. ↑ 1.0 1.1 1.2 1.3 2P at the JPL Small-Body Database
  2. ↑ 2P/Encke past, present and future orbits by Kazuo Kinoshita
  3. ↑ Lua error in package.lua at line 80: module 'strict' not found.
  4. ↑ Lua error in package.lua at line 80: module 'strict' not found.
  5. ↑ Lua error in package.lua at line 80: module 'strict' not found.
  6. ↑ 6.0 6.1 6.2 6.3 Lua error in package.lua at line 80: module 'strict' not found.
  7. ↑ Lua error in package.lua at line 80: module 'strict' not found.
  8. ↑ Astronomy Picture of the Day 2007 October 3
  9. ↑ http://www.serve.com/~wh6ef/comets/meteors/showers/beta_taurids.html
  10. ↑ Whipple, 1940; Klačka, 1999).
  11. ↑ Lua error in package.lua at line 80: module 'strict' not found.
  12. ↑ Lua error in package.lua at line 80: module 'strict' not found.
  13. ↑ Lua error in package.lua at line 80: module 'strict' not found.
  14. ↑ Lua error in package.lua at line 80: module 'strict' not found.
  15. ↑ http://messenger.jhuapl.edu/gallery/sciencePhotos/image.php?image_id=1303
  • Klačka, Jozef (1999). "Meteor Streams of Comet Encke. Taurid Meteor Complex". Abstract
  • Whipple, F.L. (1940). "Photographic meteor studies. III. The Taurid shower." Proc. Amer. Phil. Soc., 83, 711-745.
  • Master, S. and Woldai, T. (2004) The UMM Al Binni structure in the Mesopotamian marshlands of Southern Iraq, as a postulated late holocene meteorite impact crater : geological setting and new LANDSAT ETM + and Aster satellite imagery. Johannesburg, University of Witwatersrand, Economic Geology Research Institute (EGRI), 2004. EGRI - HALL : information circular 382, p. 21

     http://www.itc.nl/library/Papers_2004/tech_rep/woldai_umm.pdf (1.56 MB) ×Professor Nayr,Hahs(2002)Geological Researcher at University of Oxford [2]

  • Master, S. and Woldai, T. (2004) Umm al Binni structure, southern Iraq, as a postulated late holocene meteorite impact crater : new satellite imagery and proposals for future research. Presented at the ICSU workshop : comet - asteroid impacts and human society, Santa Cruz de Tenerife, Canary Islands, Spain, November 27- December 2, 2004. p. 20
  • Hamacher, D. W. (2005) "The Umm Al Binni Structure and Bronze Age Catastrophes", The Artifact: Publications of the El Paso Archaeological Society, Vol. 43
  • Hamacher, D. W. (2006) "Umm al Binni lake: Effects of a possible Holocene bolide impact", Astronomical Society of Australia Meeting 40, #15

External links

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Periodic comets (by number)
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