Svoboda | Graniru | BBC Russia | Golosameriki | Facebook

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
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

From Wikipedia, the free encyclopedia

HD 11506 b
Discovery
Discovered byFischer et al.
Discovery siteCalifornia,  United States
Discovery dateApril 10, 2007
Radial velocity
Orbital characteristics[1]
2.800+0.123
−0.136
 AU
Eccentricity0.391±0.010
4.418 ± 0.012 years (1,613.7 ± 4.4 d)
Inclination112.598°+23.304°
−52.700°
80.266°+23.453°
−41.201°
2451787.838+16.442
−12.388
217.469°+2.387°
−2.314°
Semi-amplitude78.402+1.408
−1.146
 m/s
StarHD 11506
Physical characteristics[1]
Mass4.880+1.986
−0.333
 MJ

HD 11506 b is an extrasolar planet that orbits the star HD 11506 167 light years away in the constellation of Cetus. This planet was discovered in 2007 by the N2K Consortium using the Keck telescope to detect the radial velocity variation of the star caused by the planet.[2] A second planet, HD 11506 c, was discovered in 2015.[3]

In 2022, the true mass and inclination of HD 11506 b were measured via astrometry, along with the discovery of a third planet in the system.[1]

YouTube Encyclopedic

  • 1/3
    Views:
    18 202
    2 357
    368 178
  • RBI Grade B Preparation - तैयारी कैसे शुरू करे
  • How Does an Egg Make an Organism? with John Gurdon
  • Britain’s Dangerous motorcycle gangs BBC Documentary 2016 (HD) #Bikelife

Transcription

See also

References

  1. ^ a b c Feng, Fabo; Butler, R. Paul; et al. (August 2022). "3D Selection of 167 Substellar Companions to Nearby Stars". The Astrophysical Journal Supplement Series. 262 (21): 21. arXiv:2208.12720. Bibcode:2022ApJS..262...21F. doi:10.3847/1538-4365/ac7e57. S2CID 251864022.
  2. ^ Fischer, Debra A.; et al. (2007). "Five Intermediate-Period Planets from the N2K Sample". The Astrophysical Journal. 669 (2): 1336–1344. arXiv:0704.1191. Bibcode:2007ApJ...669.1336F. doi:10.1086/521869. S2CID 7774321.
  3. ^ Giguere, Matthew J.; et al. (2015). "Newly Discovered Planets Orbiting HD 5319, HD 11506, HD 75784 and HD 10442 from the N2K Consortium". The Astrophysical Journal. 799 (1). 89. arXiv:1411.5374. Bibcode:2015ApJ...799...89G. doi:10.1088/0004-637X/799/1/89. S2CID 56121568.


This page was last edited on 27 November 2023, at 23:51
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.