Comets are icy objects that release gas and dust as they orbit the Sun. The solid part of a comet is called the nucleus and is mainly made of frozen water, dust and sometimes other frozen substances such as ammonia.
Solar radiation heats the nucleus and gives it an atmosphere of gas and dust called the coma. A comet's distinctive tail is caused by solar radiation and a stream of charged particles that constantly jets away from the Sun called the solar wind.
It is thought that comets are material leftover from the formation of the outer planets, although another theory is that many formed outside our solar system.
Photo: Comet Holmes taken by the Spitzer Space Telescope (NASA)
Leftover building material orbits the Sun.
The comet's impact shows planet building in action.
The comet Shoemaker-Levy 9 struck Jupiter on 16 July 1994. Clearly visible through telescopes on Earth, the impact was the first time a collision between two objects in the Solar System had been seen. Researchers believe that the planets formed through a series of such collisions. This clip features commentary by Dr David Levy, co-discoverer of Shoemaker-Levy 9.
Patrick Moore talks about the amazing light show that takes place every August.
Patrick Moore talks to guest Dr John Mason about the Perseid meteor shower that takes place every August when the Earth passes through the dust and gas trail left by Comet Swift-Tuttle. In 2007 when this interview took place visibility was very good but cloud cover and the Moon can get in the way.
Volcanoes and comets bring water to the Earth.
Dr Iain Stewart explains the theory that steam from volcanoes and water from comets filled the Earth's oceans.
The Vega probes give astronomers a close-up look at the comet.
In 1986 the Russian Vega probes captured close-up images of Halley's comet in preparation for the European Giotto probe.
Patrick Moore and his guest discuss the comet's collision with Jupiter.
Sir Patrick Moore and his guest Dr Steven Miller discuss the comet's collision with Jupiter.
A comet is an icy small Solar System body that, when passing close to the Sun, heats up and begins to outgas, displaying a visible atmosphere or coma, and sometimes also a tail. These phenomena are due to the effects of solar radiation and the solar wind upon the nucleus of the comet. Comet nuclei range from a few hundred metres to tens of kilometres across and are composed of loose collections of ice, dust, and small rocky particles. The coma and tail are much larger and, if sufficiently bright, may be seen from the Earth without the aid of a telescope. Comets have been observed and recorded since ancient times by many different cultures.
Comets have a wide range of orbital periods, ranging from several years to several millions of years. Short-period comets originate in the Kuiper belt or its associated scattered disc, which lie beyond the orbit of Neptune. Longer-period comets are thought to originate in the Oort cloud, a spherical cloud of icy bodies extending from outside the Kuiper Belt to halfway to the next nearest star. Long-period comets are directed towards the Sun from the Oort cloud by gravitational perturbations caused by passing stars and the galactic tide. Hyperbolic comets may pass once through the inner Solar System before being flung out to interstellar space along hyperbolic trajectories.
Comets are distinguished from asteroids by the presence of an extended, gravitationally unbound atmosphere surrounding their central nucleus. This atmosphere has parts termed the coma (the central atmosphere immediately surrounding the nucleus) and the tail (a typically linear section consisting of dust or gas blown out from the coma by the Sun's light pressure or outstreaming solar wind plasma). However, extinct comets that have passed close to the Sun many times have lost nearly all of their volatile ices and dust and may come to resemble small asteroids. Asteroids are thought to have a different origin from comets, having formed inside the orbit of Jupiter rather than in the outer Solar System. The discovery of main-belt comets and active centaurs has blurred the distinction between asteroids and comets.
As of August 2014[update] there are 5,186 known comets, a number which is steadily increasing. However, this represents only a tiny fraction of the total potential comet population, as the reservoir of comet-like bodies in the outer Solar System may number one trillion. Roughly one comet per year is visible to the naked eye, though many of these are faint and unspectacular. Particularly bright examples are called "Great Comets".
On 22 January 2014, ESA scientists reported the detection, for the first definitive time, of water vapor on the dwarf planet Ceres, the largest object in the asteroid belt. The detection was made by using the far-infrared abilities of the Herschel Space Observatory. The finding is unexpected because comets, not asteroids, are typically considered to "sprout jets and plumes". According to one of the scientists, "The lines are becoming more and more blurred between comets and asteroids." On 11 August 2014, astronomers released studies, using the Atacama Large Millimeter/Submillimeter Array (ALMA) for the first time, that detailed the distribution of HCN, HNC, H2CO, and dust inside the comae of comets C/2012 F6 (Lemmon) and C/2012 S1 (ISON).