To install click the Add extension button. That's it.

The source code for the WIKI 2 extension is being checked by specialists of the Mozilla Foundation, Google, and Apple. You could also do it yourself at any point in time.

4,5
Kelly Slayton
Congratulations on this excellent venture… what a great idea!
Alexander Grigorievskiy
I use WIKI 2 every day and almost forgot how the original Wikipedia looks like.
Live Statistics
English Articles
Improved in 24 Hours
Added in 24 Hours
Languages
Recent
Show all languages
What we do. Every page goes through several hundred of perfecting techniques; in live mode. Quite the same Wikipedia. Just better.
.
Leo
Newton
Brights
Milds

N2K Consortium

From Wikipedia, the free encyclopedia

The N2K Consortium is a collaborative multinational effort by American, Chilean and Japanese astronomers to find additional extrasolar planets around stars that are not already being surveyed. The N2K is shorthand for the set of roughly 2,000 of the nearest and most luminous main sequence stars that were selected to be newly surveyed. Target stars have a B - V color index value between 0.4 and 1.2, a visual magnitude brighter than 10.5, and a distance of less than 110 pc from the Sun. They were selected based upon their high metallicity, which is the abundance of elements other than hydrogen and helium.[1]

The observing campaign uses the Keck, Magellan and Subaru telescopes, plus automated telescopes at Fairborn Observatory. Each star is observed three times over a period of several days, then checked for short period variations in radial velocity. This variation is a characteristic of gravitational perturbation caused by a hot Jupiter. Those stars showing radial velocity variations are then checked with the automated photometric telescopes from Fairborn Observatory.[1]

During a two-year run beginning in 2004, the N2K Consortium was predicted to detect about 60 new hot Jupiters.[1] However, by 2009, only seven planets with orbital periods of up to five days had been discovered. They orbit the following stars:[2]

See also

References

  1. ^ a b c d Fischer, Debra A.; et al. (2005). "The N2K Consortium. I. A Hot Saturn Planet Orbiting HD 88133" (PDF). The Astrophysical Journal. 620 (1): 481. Bibcode:2005ApJ...620..481F. doi:10.1086/426810.
  2. ^ Sato, Bun'ei; et al. (September 2009). "A Substellar Companion in a 1.3 yr Nearly Circular Orbit of HD 16760". The Astrophysical Journal. 703 (1): 671–674. arXiv:0907.5080. Bibcode:2009ApJ...703..671S. doi:10.1088/0004-637X/703/1/671. S2CID 5435270.
  3. ^ a b Fischer, Debra A.; et al. (2006). "The N2K Consortium. III. Short-Period Planets Orbiting HD 149143 and HD 109749". The Astrophysical Journal. 637 (2): 1094–1101. Bibcode:2006ApJ...637.1094F. doi:10.1086/498557.

External links

This page was last edited on 19 August 2023, at 03:28
Basis of this page is in Wikipedia. Text is available under the CC BY-SA 3.0 Unported License. Non-text media are available under their specified licenses. Wikipedia® is a registered trademark of the Wikimedia Foundation, Inc. WIKI 2 is an independent company and has no affiliation with Wikimedia Foundation.