Home  

Random  

Nearby  



Log in  



Settings  



Donate  



About Wikipedia  

Disclaimers  



Wikipedia





Talk:Kepler-47





Article  

Talk  



Language  

Watch  

Edit  


Latest comment: 1 year ago by SevenSpheres in topic Surface gravity
 


Learn more about this page

Found star data finally

edit

examiner.com/article/the-nature-of-the-kepler-47-system

http://www.openexoplanetcatalogue.com/system.html?id=Kepler-47(AB)%20b

On Wednesday, astronomers announced the discovery of two planets orbiting a binary star system known as Kepler-47. The star is 1,500 parsecs away from Earth, and is the first binary star system that has been found to have more than one planet. The two planets were discovered by NASA's Kepler space telescope, which has spotted 77 exoplanets and 2,321 exoplanet candidates since it was launched in March 2009.

Kepler-47 is in the constellation Cygnus. The two stars are known as Kepler-47A and Kepler-47B, and they orbit each other every 7.45 Earth days.

Kepler-47A has 1.043±0.055 times the mass of the Sun and 0.964±0.017 times the radius of the Sun. Its mean surface temperature is estimated to be 5636±100 K, while the mean surface temperature of the Sun is 5778 K. The spectral classification of Kepler-47A is G6V, which is slightly dimmer and redder than the G2V spectral classification of the Sun.

Kepler-47B has 0.362±0.013 times the mass of the Sun and 0.3506±0.0063 times the radius of the Sun. Its mean surface temperature is estimated to be 3357±100 K. The spectral classification of Kepler-47B is M4V, making it a red dwarf star.

Star Mass
(sol)
Radius
(sol)
Effective
Temperatre(K)
Mass
(Mj)
Radius
(Mj)
Semi-Major
Axis (AU)
Irradiance
(W/m2)
Irradiance
(% of Sol)
Irradiance
(% Total)
Effective
Temperature (°C)
Kepler-47A 1.043±0.055 0.964±0.017 5636±100 K
Kepler-47B 0.362±0.013 0.3506±0.0063 3357±100 K
Kepler-47A-b 2.7 0.265 0.2956±0.0047 13152.09 962.76%
Kepler-47B-b 2.7 0.265 0.2956±0.0047 218.97 16.03% 978.79% 175.85
Kepler-47A-c 17 0.410 0.989±0.016 1174.93 86.01%
Kepler-47B-c 17 0.410 0.989±0.016 19.56 1.43% 87.44% -28.15
Earth/Sun 1 1 5778 0.00315 0.0892 1 1366.08 100% -18


=((((695500000)*0.964)^2)*(0.0000000567051)*(5636^4))/(149597870690*0.989)^2 = 13152.09 W/m2

24.79.40.8 (talk) 22:47, 10 September 2013 (UTC)Reply

at least three planets?

edit

Lede states there are "at least three planets" then goes on to talk about "the two planets". Inconsistency is obvious. Qemist (talk) 06:31, 26 April 2014 (UTC)Reply

Surface gravity

edit

Why is the surface gravity of Kepler-47B bigger than that of Kepler-47A, while the former is less massive? Aminabzz (talk) 17:34, 12 May 2023 (UTC)Reply

Because star B is significantly more dense than star A. SevenSpheres (talk) 19:37, 12 May 2023 (UTC)Reply
Newton himself gave us a formula for gravity and it just has mass and distance. Volume and density are irrelevant. Aminabzz (talk) 22:10, 18 May 2023 (UTC)Reply
This is specifically the surface gravity. Kepler-47A indeed has a greater gravitational force on an object at a given distance from it than Kepler-47B has on an object at the same distance, but since Kepler-47A is larger, its surface is farther from its center of mass and so the gravity at its surface is (slightly) less than that of Kepler-47B. SevenSpheres (talk) 21:58, 20 May 2023 (UTC)Reply

Add topic

Retrieved from "https://en.wikipedia.org/w/index.php?title=Talk:Kepler-47&oldid=1202941031"
 



Last edited on 3 February 2024, at 21:42  


Languages

 



This page is not available in other languages.
 

Wikipedia


This page was last edited on 3 February 2024, at 21:42 (UTC).

Content is available under CC BY-SA 4.0 unless otherwise noted.



Privacy policy

About Wikipedia

Disclaimers

Contact Wikipedia

Code of Conduct

Developers

Statistics

Cookie statement

Terms of Use

Desktop