Comet NEAT (disambiguation)

Last updated

Comet NEAT may refer to any comets below discovered by the Near-Earth Asteroid Tracking survey:

Contents

Periodic comets

180P/NEAT 180P 2023-02-19 image ZTF-sso-710-zr-size-5.0arcmin.png
180P/NEAT
207P/NEAT 207P 2024-03-05 image ZTF-sso-357-zg-size-600.0arcsec.png
207P/NEAT
240P/NEAT 240P 2018-12-12 image ZTF-sso-669-zr-fov-7.0arcmin.png
240P/NEAT
246P/NEAT 246P 2021-06-08 image ZTF-sso-236-zr-fov-9.3arcmin.png
246P/NEAT

Jupiter-family comets

Halley-type comets

Chiron-type comets

Non-Periodic comets

C/2002 V1 C 2002 V1 2003-02-01 J87 v1.jpg
C/2002 V1

Hyperbolic comets

C/2001 Q4 Comet-Neat-Messier-44 log.jpg
C/2001 Q4

Others

54P/de Vico-Swift-NEAT Comet de Vico-Swift 1965 (US Navy).jpg
54P/de Vico–Swift–NEAT
193P/LINEAR-NEAT 193P 2021-09-10 image ZTF-sso-445-zr-fov-7.0arcmin.png
193P/LINEAR–NEAT
395P/Catalina-NEAT 395P 2022-09-04 image ZTF-sso-445-zr-fov-5.6arcmin.png
395P/Catalina–NEAT

"Comet NEAT" may also be an incomplete reference to a comet co-discovered by the Near-Earth Asteroid Tracking survey. These include:


Related Research Articles

<span class="mw-page-title-main">Asteroid impact avoidance</span> Methods to prevent destructive asteroid hits

Asteroid impact avoidance encompasses the methods by which near-Earth objects (NEO) on a potential collision course with Earth could be diverted away, preventing destructive impact events. An impact by a sufficiently large asteroid or other NEOs would cause, depending on its impact location, massive tsunamis or multiple firestorms, and an impact winter caused by the sunlight-blocking effect of large quantities of pulverized rock dust and other debris placed into the stratosphere. A collision 66 million years ago between the Earth and an object approximately 10 kilometers wide is thought to have produced the Chicxulub crater and triggered the Cretaceous–Paleogene extinction event that is understood by the scientific community to have caused the extinction of all non-avian dinosaurs.

<span class="mw-page-title-main">Lincoln Near-Earth Asteroid Research</span> American astronomical survey for identifying and tracking near-Earth objects

The Lincoln Near-Earth Asteroid Research (LINEAR) project is a collaboration of the United States Air Force, NASA, and the Massachusetts Institute of Technology's Lincoln Laboratory for the systematic detection and tracking of near-Earth objects. LINEAR was responsible for the majority of asteroid discoveries from 1998 until it was overtaken by the Catalina Sky Survey in 2005. As of 15 September 2011, LINEAR had detected 231,082 new small Solar System bodies, of which at least 2,423 were near-Earth asteroids and 279 were comets. The instruments used by the LINEAR program are located at Lincoln Laboratory's Experimental Test Site (ETS) on the White Sands Missile Range (WSMR) near Socorro, New Mexico.

Near-Earth Asteroid Tracking (NEAT) was a program run by NASA and the Jet Propulsion Laboratory, surveying the sky for near-Earth objects. NEAT was conducted from December 1995 until April 2007, at GEODSS on Hawaii, as well as at Palomar Observatory in California. With the discovery of more than 40 thousand minor planets, NEAT has been one of the most successful programs in this field, comparable to the Catalina Sky Survey, LONEOS and Mount Lemmon Survey.

Damocloids are a class of minor planets such as 5335 Damocles and 1996 PW that have Halley-type or long-period highly eccentric orbits typical of periodic comets such as Halley's Comet, but without showing a cometary coma or tail. David Jewitt defines a damocloid as an object with a Jupiter Tisserand invariant (TJ) of 2 or less, while Akimasa Nakamura defines this group with the following orbital elements:

<span class="mw-page-title-main">Lewis A. Swift</span> American astronomer (1820–1913)

Lewis A. Swift was an American astronomer who discovered 13 comets and 1,248 previously uncatalogued nebulae. Only William Herschel discovered more nebulae visually.

<span class="mw-page-title-main">Lowell Observatory Near-Earth-Object Search</span> 1993–2008 research project

Lowell Observatory Near-Earth-Object Search (LONEOS) was a project designed to discover asteroids and comets that orbit near the Earth. The project, funded by NASA, was directed by astronomer Ted Bowell of Lowell Observatory in Flagstaff, Arizona. The LONEOS project began in 1993 and ran until the end of February 2008.

<span class="mw-page-title-main">Catalina Sky Survey</span> Project to discover comets, asteroids, and near-Earth objects

Catalina Sky Survey is an astronomical survey to discover comets and asteroids. It is conducted at the Steward Observatory's Catalina Station, located near Tucson, Arizona, in the United States.

Edward L. G. "Ted" Bowell, was an American astronomer. Bowell was educated at Emanuel School London, University College, London, and the University of Paris.

Roy A. Tucker (1951 – 2021) was an American astronomer best known for the co-discovery of near-Earth asteroid 99942 Apophis (formerly known as 2004 MN4) along with David J. Tholen and Fabrizio Bernardi of the University of Hawaii. He was a prolific discoverer of minor planets, credited by the Minor Planet Center with the discovery of 702 numbered minor planets between 1996 and 2010. He also discovered two comets: 328P/LONEOS–Tucker and C/2004 Q1, a Jupiter-family and near-parabolic comet, respectively.

Robert H. McNaught is a Scottish-Australian astronomer at the Research School of Astronomy and Astrophysics of the Australian National University (ANU). He has collaborated with David J. Asher of the Armagh Observatory.

The Palomar Planet-Crossing Asteroid Survey (PCAS) was an astronomical survey, initiated by American astronomers Eleanor Helin and Eugene Shoemaker at the U.S Palomar Observatory, California, in 1973. The program is responsible for the discovery of 95 near-Earth Objects including 17 comets, while the Minor Planet Center directly credits PCAS with the discovery of 20 numbered minor planets during 1993–1994. PCAS ran for nearly 25 years until June 1995. It had an international extension, INAS, and was the immediate predecessor of the outstandingly successful NEAT program.

<span class="mw-page-title-main">596 Scheila</span> Main-belt asteroid

596 Scheila is a main-belt asteroid and main-belt comet orbiting the Sun. It was discovered on 21 February 1906 by August Kopff from Heidelberg. Kopff named the asteroid after a female English student with whom he was acquainted.

James Whitney Young is an American astronomer who worked in the field of asteroid research. After nearly 47 years with the Jet Propulsion Laboratory at their Table Mountain Facility, Young retired July 16, 2009.

<span class="mw-page-title-main">166P/NEAT</span> Periodic comet with 51 year orbit

166P/NEAT is a periodic comet and centaur in the outer Solar System. It was discovered by the Near Earth Asteroid Tracking (NEAT) project in 2001 and initially classified a comet with provisional designation P/2001 T4 (NEAT), as it was apparent from the discovery observations that the body exhibited a cometary coma. It is one of few known bodies with centaur-like orbits that display a coma, along with 60558 Echeclus, 2060 Chiron, 165P/LINEAR and 167P/CINEOS. It is also one of the reddest centaurs.

<span class="mw-page-title-main">C/2001 Q4 (NEAT)</span> Hyperbolic comet

C/2001 Q4 (NEAT) is a comet with an almost perpendicular retrograde orbit which brings it into the inner Solar System by a deeply southward path. It initially emerged from its remote home spending most of its time near the south celestial pole. This comet was discovered on August 24, 2001 by the Near-Earth Asteroid Tracking program (NEAT).

<span class="mw-page-title-main">54P/de Vico–Swift–NEAT</span> Periodic comet with 7 year orbit

54P/de Vico–Swift–NEAT is a periodic comet in the Solar System first discovered by Father Francesco de Vico on August 23, 1844. It has become a lost comet several times after its discovery. The comet makes many close approaches to Jupiter. The comet was last observed on 20 December 2009 by Ageo Observatory.

<span class="mw-page-title-main">Extinct comet</span> Comet that lacks typical activity

An extinct comet is a comet that has expelled most of its volatile ice and has little left to form a tail and coma. In a dormant comet, rather than being depleted, any remaining volatile components have been sealed beneath an inactive surface layer.

C/2001 OG108 (LONEOS) is a Halley-type comet with an orbital period of 48.51 years. It was discovered on 28 July 2001 by the LONEOS telescope at Lowell Observatory. Of the short-period comets with known diameters and perihelion inside the orbit of Earth, C/2001 OG108 is the second largest after Comet Swift–Tuttle.

Eric James Christensen is an American astronomer and a discoverer of comets. Since 2023, he works as an Observing Specialist Manager at the Vera C. Rubin Observatory. Before this, he was a staff scientist with the Catalina Sky Survey (CSS), where he was responsible for the survey's near-Earth object operation.

<span class="mw-page-title-main">Comet Swift</span> Index of articles associated with the same name

Comet Swift or Swift's Comet, may refer to any of the 9 comets discovered by American astronomer, Lewis A. Swift, below: