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

HAT-P-9b / Alef
Size comparison of HAT-P-9b with Jupiter.
Discovery
Discovered byShporer et al.
Discovery siteCambridge, Massachusetts
Discovery dateJune 26, 2008
Transit (SuperWASP)
Orbital characteristics
0.0528 ± 0.002 AU (7,900,000 ± 300,000 km)
Eccentricity~0.0012
3.92289 ± 0.00004 d
StarHAT-P-9
Physical characteristics
Mean radius
1.4 ± 0.06 RJ
Mass0.78 ± 0.09 MJ
Mean density
380 kg/m3 (640 lb/cu yd)
10.3 m/s2 (34 ft/s2)
1.05 g

HAT-P-9b, formally named Alef,[1] is an exoplanet approximately 1500 light years away in the constellation Auriga. This planet was found by the transit method on June 26, 2008. It has a mass 78% that of Jupiter and a radius 140% that of Jupiter. As with most transiting planets, this planet is a hot Jupiter, meaning this Jupiter-like planet orbits extremely close to its parent star, taking only 3.92 days to orbit.[2]

The study in 2012, utilizing a Rossiter–McLaughlin effect, have determined the planetary orbit is mildly misaligned with the rotational axis of the star, misalignment equal to -16±8°.[3]

The name Alef was selected in the NameExoWorlds campaign by Israel, during the 100th anniversary of the IAU. Alef is the first letter in the Hebrew alphabet and also means bull.[1]

YouTube Encyclopedic

  • 1/1
    Views:
    4 408
  • Expected Questions on Space Research: UPSC IAS Prelims & Mains 2017

Transcription

References

  1. ^ a b "Approved names". NameExoworlds. Retrieved 2020-01-02.
  2. ^ Shporer, Avi; et al. (2009). "HAT-P-9b: A Low-Density Planet Transiting a Moderately Faint F Star". The Astrophysical Journal. 690 (2): 1393–1400. arXiv:0806.4008. Bibcode:2009ApJ...690.1393S. doi:10.1088/0004-637X/690/2/1393. S2CID 930937.
  3. ^ Albrecht, Simon; Winn, Joshua N.; Johnson, John A.; Howard, Andrew W.; Marcy, Geoffrey W.; Butler, R. Paul; Arriagada, Pamela; Crane, Jeffrey D.; Shectman, Stephen A.; Thompson, Ian B.; Hirano, Teruyuki; Bakos, Gaspar; Hartman, Joel D. (2012), "Obliquities of Hot Jupiter host stars: Evidence for tidal interactions and primordial misalignments", The Astrophysical Journal, 757 (1): 18, arXiv:1206.6105, Bibcode:2012ApJ...757...18A, doi:10.1088/0004-637X/757/1/18, S2CID 17174530

External links

Media related to HAT-P-9b at Wikimedia Commons



This page was last edited on 20 August 2023, at 16:29
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.