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Subaru Telescope reveals the shape and temperature of Comet Encke's nucleus
explained
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. 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 its 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 its nucleus receives, although comets generate a large coma and tail that can make them much more visible during their perihelion (closest approach to the Sun). The diameter of the nucleus of Encke's Comet is 4.86 km (3.02 mi).
It reaches opposition on 8 October 2026 when it will be about magnitude 15. It comes to perihelion on 10 February 2027 when it will have a solar elongation of 10 degrees.
From Wikipedia: Comet Encke (CC BY-SA 4.0) ↗Sunlight heats the nucleus and it re-emits that energy as infrared. The emission depends on the surface area facing us and on temperature, so as the comet spins, the changing infrared brightness reveals its shape.
A comet's nucleus is usually too small and too far away to see directly, so its size and temperature have to be inferred from heat. Those numbers show how fast it loses ice and how long it can survive.
The meteor showers known as the Taurids are linked to debris from Encke.
Illustrative photo · Jim Scotti, Public domain, via Wikimedia Commons
