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Past, current, and pending searches for Nemesis
Searches for Nemesis in the infrared are important because cooler stars comparatively shine brighter in infrared light. The University of California
The University of California (UC) is a public land-grant research university system in the U.S. state of California. The system is composed of the campuses at Berkeley, Davis, Irvine, Los Angeles, Merced, Riverside, San Diego, San Franci ...
's Leuschner Observatory
Leuschner Observatory, originally called the Students' Observatory, is an observatory jointly operated by the University of California, Berkeley and San Francisco State University. The observatory was built in 1886 on the Berkeley campus. For many ...
failed to discover Nemesis by 1986. The Infrared Astronomical Satellite ( IRAS) failed to discover Nemesis in the 1980s. The 2MASS
The Two Micron All-Sky Survey, or 2MASS, was an astronomical survey of the whole sky in infrared light. It took place between 1997 and 2001, in two different locations: at the U.S. Fred Lawrence Whipple Observatory on Mount Hopkins, Arizona, and ...
astronomical survey, which ran from 1997 to 2001, failed to detect a star, or brown dwarf, in the Solar System. If Nemesis exists, it may be detected by Pan-STARRS
The Panoramic Survey Telescope and Rapid Response System (Pan-STARRS1; obs. code: F51 and Pan-STARRS2 obs. code: F52) located at Haleakala Observatory, Hawaii, US, consists of astronomical cameras, telescopes and a computing facility that is ...
or the planned LSST astronomical surveys.
In particular, if Nemesis is a red dwarf or a brown dwarf
Brown dwarfs (also called failed stars) are substellar objects that are not massive enough to sustain nuclear fusion of ordinary hydrogen ( 1H) into helium in their cores, unlike a main-sequence star. Instead, they have a mass between the most ...
, the WISE mission (an infrared sky survey that covered most of the solar neighborhood in movement-verifying parallax measurements) was expected to be able to find it. WISE can detect 150-kelvin brown dwarfs out to 10 light-years, and the closer a brown dwarf is, the easier it is to detect. Preliminary results of the WISE survey were released on April 14, 2011.[ On March 14, 2012, the entire catalog of the WISE mission was released.] In 2014 WISE data ruled out a Saturn or larger-sized body in the Oort cloud out to ten thousand AU.NASA's WISE Survey Finds Thousands of New Stars, But No 'Planet X'
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Calculations in the 1980s suggested that a Nemesis object would have an irregular orbit due to perturbations from the galaxy and passing stars. The Melott and Bambach work shows an extremely regular signal, inconsistent with the expected irregularities in such an orbit. Thus, while supporting the extinction periodicity, it appears to be inconsistent with the Nemesis hypothesis, though of course not inconsistent with other kinds of substellar objects. According to a 2011 NASA news release, "recent scientific analysis no longer supports the idea that extinctions on Earth happen at regular, repeating intervals, and thus, the Nemesis hypothesis is no longer needed."
See also
* Giant impact hypothesis
* Lists of astronomical objects
* Malmquist bias
* Planet Nine
* Planets beyond Neptune
Following the discovery of the planet Neptune in 1846, there was considerable speculation that another planet might exist beyond its orbit. The search began in the mid-19th century and continued at the start of the 20th with Percival Lowell's ...
* Shiva hypothesis
The Shiva hypothesis, also known as coherent catastrophism, is the idea that global natural catastrophes on Earth, such as extinction events, happen at regular intervals because of the periodic motion of the Sun in relation to the Milky Way galax ...
* Theia (planet)
Theia is a hypothesized ancient planet in the early Solar System that, according to the giant-impact hypothesis, collided with the early Earth around 4.5 billion years ago, with some of the resulting ejected debris gathering to form the Moon.
...
* Tyche (hypothetical planet)
* Vulcan (hypothetical planet)
Vulcan was a theorized planet that some pre-20th century astronomers thought existed in an orbit between Mercury and the Sun. Speculation about, and even purported observations of, intermercurial bodies or planets date back to the beginning o ...
References
External links
"Astrobiology Magazine", "Cosmic Evolution" Section, "Getting WISE about Nemesis"
03/11/10, Author: Leslie Mullen, Article about Nemesis and Tyche theory, and how the WISE Sky Survey Mission may prove or disprove the theories.
* Robert Roy Britt,
', Space.com, 3 April 2001.
*
* Richard A. Muller,
Measurement of the lunar impact record for the past 3.5 billion years, and implications for the Nemesis theory
', Geological Society of America Special Paper 356, pp 659–665 (2002). I
* Richard A. Muller
(Weidenfeld & Nicolson, 1988, OP)
* Richard A. Muller, lecture where he describe
Nemesis Theory
* Z.K. Silagadze,
TeV scale gravity, mirror universe, and ... dinosaurs
'
Acta Physica Polonica
B32 (2001) 99–128. ''(Provides a very entertaining and readable review of the Nemesis extinction hypothesis, including dozens of references to scientific articles on the topic.)''
* SpaceDaily
Apr 25, 2006
* Lynn Yarris. "Does a Companion Star to the Sun Cause Earth's Periodic Mass Extinctions?" Science Beat. Spring 1987
Nemesis is a myth
(Max Planck August 1, 2011)
{{DEFAULTSORT:Nemesis (Star)
Hypothetical bodies of the Solar System
Hypothetical stars
Theories
Solar System dynamic theories
M-type main-sequence stars
Brown dwarfs
Extinction events
Hypothetical trans-Neptunian objects
Oort cloud
Cosmic doomsday
Obsolete theories in physics