Comet Encke
Comet Encke or Encke's Comet is a periodic comet that completes an orbit of the Sun once every 3.3 years. Encke was first recorded by Pierre Méchain on 17 January 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 when talking about the nucleus. However, comets generate a large coma and tail that can make them much more visible during their perihelion. The diameter of the nucleus of Encke's Comet is 4.8 km.
Discovery
As its official designation implies, Encke's Comet was the first periodic comet discovered after Halley's Comet. It was independently observed by several astronomers, the first two being Pierre Méchain and Charles Messier in 1786. It was next observed by Caroline Herschel in 1795 and was "discovered" for a third time by Jean-Louis Pons in 1818. Its orbit was calculated by Johann Franz Encke, who through laborious calculations was able to link observations of comets in 1786, 1795, 1805 and 1818 to the same object. In 1819 he published his conclusions in the journal Correspondance astronomique, and predicted correctly its return in 1822. It was recovered by Carl Ludwig Christian Rümker at Parramatta Observatory on 2 June 1822.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. Encke is currently close to a 7:2 mean motion resonance with Jupiter, and it is possible that some of the larger fragments shed by the comet, or released by a larger progenitor of the comet, are trapped in this resonance.Encke's orbit gets as close as to Earth. 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. On 18 November 2013, it passed from Mercury. Close approaches to Earth usually occur every 33 years.
Observations
The comet has been observed at every perihelion since 1818 except 1944.An attempt to photograph the comet close to aphelion was made on 2 July 1913 using the Mount Wilson 60-inch telescope but the resulting photographic plate was lost in the mail. A second attempt using the same telescope was made on 1 September 1913 and this showed an object in about the right position but orbital uncertainties made it impossible to be sure of its identity.
In March 1918 the Greenwich 28-inch aperture telescope took observations Encke.
An observer of Encke's in March 1918 had this to say of the comet on March 12, comparing to the early March 9 observation, "The comet much shaper, brighter, smaller; its diameter was 1 1/2', magnitude 7.7. Its magnitude in the 6-inch Corbett was almost stellar, but in the 28 inch no definitive nucleus could be seen."
The failed CONTOUR mission was launched to study this comet, and also Schwassmann-Wachmann 3.
loses its tail
On 20 April, 2007, STEREO-A observed the tail of Comet Encke to be temporarily torn off by magnetic field disturbances caused by a coronal mass ejection. The tail grew back due to the continuous shedding of dust and gas by the comet.
Meteor showers
Comet Encke is believed to be the originator of several related meteor showers known as the Taurids. A shower has similarly been reported affecting Mercury.Near-Earth object may be a fragment of Encke.
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 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 particles 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.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, may have been caused by the impact of a cometary body, has also been postulated by Czechoslovakian astronomer Ľubor Kresák as a fragment of Comet Encke.
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. Comet Encke has sometimes been identified as the comet in question. In their 1982 book Cosmic Serpent 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 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.
Astronomers planned a 2019 search campaign for fragments of comet Encke which would have been visible from Earth as the Taurid swarm passed between July 5–11, and July 21 – August 10. There were no reports of discoveries of any such objects.
Importance in the scientific history of luminiferous aether
Comet Encke 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 reads:Encke's pole tumbles in an 81-year period, therefore it will accelerate for half that time, and decelerate for the other half of the time,. The authors of this 1860 textbook of course could not know that the pole of the comet would tumble as it does over such a long period of time, or that outgassing would induce a thrust to change its course.