Current status of HZ exoplanets. This gives the results of…
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Current status of HZ exoplanets.
This gives the results of the known (confirmed) exoplanets (8,177) in their respective HZ. The table shows the hot to cold zones (color), stellar host star type, and three size ranges. "Earthish" size is 0.4 to 2.5 R; "Tiny" is < 0.4R; and "Big" is > 2.5R. \HZ exoplanets found in their HZ but their radius is still unknown are also listed.\]
My hope is to find a nice way to give detailed information on the current status of exoplanets. My program does take other important determining factors into account. (e.g. eccentricity).
I have a table of exoplanets listed by star type and luminosity zone (color), as well as, their tidal-lock status, which I'll likely post soon.
I'm not an astronomer, but I think it is quite accurate based on the current equations for HZs. Both the Temperature Equilibrium model is used and the Optimistic (Early Venus) model is used, with the latter shown in the illustration.
Data courtesy of [ exoplanet.eu http://exoplanet.eu
#space
source
This gives the results of the known (confirmed) exoplanets (8,177) in their respective HZ. The table shows the hot to cold zones (color), stellar host star type, and three size ranges. "Earthish" size is 0.4 to 2.5 R; "Tiny" is < 0.4R; and "Big" is > 2.5R. \HZ exoplanets found in their HZ but their radius is still unknown are also listed.\]
My hope is to find a nice way to give detailed information on the current status of exoplanets. My program does take other important determining factors into account. (e.g. eccentricity).
I have a table of exoplanets listed by star type and luminosity zone (color), as well as, their tidal-lock status, which I'll likely post soon.
I'm not an astronomer, but I think it is quite accurate based on the current equations for HZs. Both the Temperature Equilibrium model is used and the Optimistic (Early Venus) model is used, with the latter shown in the illustration.
Data courtesy of [ exoplanet.eu http://exoplanet.eu
#space
source
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