Exoplanet Name : |
SOI-6 b |
Alternate Name : |
|
Status : |
Confirmed |
Radius (Rjup / Re): |
0.0000 |
(Rjup) |
0.0000 |
(Rearth) |
Mass (Mjup / Me): |
0.0000 |
(Mjup) |
0.0000 |
(Mearth) |
Semi Major Axis / Orbital Distance Calculated |
0.0000 |
(AU) |
0.0000 |
(AU Est.) |
Eccentricity : |
0.6000 |
Orbital Period(Yrs) |
0.0057 |
Orbital Period(Observed/Estimated) |
2.07 |
(Days Obs.) |
0.00 |
(Days Est.) |
Surface Gravity (G Earth) |
nan |
Star Radiation at Atmospheric Boundary: |
0.0 |
(W/m2) |
Measured Temperature (K) |
0.0 |
(K) |
Blackbody T 0.1(K) |
0.0 |
(K) |
Blackbody T 0.3(K) |
0.0 |
(K) |
Blackbody T 0.7(K) |
0.0 |
(K) |
Tidally Locked Blackbody T 0.1(K) |
0.0 |
(K) |
Tidally Locked Blackbody T 0.3(K) |
0.0 |
(K) |
Size Class: |
Asteroid-size |
Mass Class: |
|
Detection Type : |
Primary Transit |
Mass Detection : |
|
Radius Detection : |
|
Habitability by Solar Eq. Astronomical Unit: |
Not habitable |
Habitability by Kopparapu: |
Not habitable |
Star Name : |
SOI-6 |
Alternate Name : |
|
Star Distance(LY) : |
0.0 |
Stellar Radius(Rsun) : |
0.6 |
(Rsun Measured) |
Stellar Mass(Msun) : |
0.0 |
(Msun Measured) |
0.0 |
(Msun Estimated) |
Star Age : |
0.0 |
(GY) |
Temperature : |
3300 |
(K) |
Spectral type : |
M9 |
UV portion[%]: |
0.2 |
Visible portion[%]: |
11.2 |
IR portion[%]: |
88.6 |
Metalicity : |
0.0 |
Absolute Magnitude: |
25.0 |
Apparent Magnitude: |
22.0 |
Right Ascension(RA) |
2.0000 |
Declination (DEC) |
50.5222 |
Hubble Space Telescope Guide Star Catalog (GSC) ID |
|
Discovered by |
|
Discovery Paper - Authors |
|
Discovery Paper - Title |
|
Discovery Paper - Journal |
|
Discovery Paper - URL |
|
SIMBAD LINK |
|
Open Exoplanet Database Link |
|
|
|
|
|
/
SOI-6 b
SOI-6 b
SOI-6 b is an exoplanet orbiting the star SOI-6. Its discovery was publicly announced on 2023.
The host star SOI-6 has apparent magnitude of 22.0, with absolute magnitude of 25.0.
In this planetary system, the extrasolar planet SOI-6 b orbits around the star SOI-6 every 2.1 days with its orbital distance of 0.00 AU ( 0.0 km)
(Projected orbit of SOI-6 b around its host star SOI-6)
The Star SOI-6 's habitable zone is located at the following distance
Inner Boundary (the orbital distance at Venus's Equivalent Radiation )
: 0.137 AU ( 20469818.2 km)
Earth Boundary (the orbital distance at Earth's Equivalent Radiation)
: 0.189 AU ( 28294638.2 km)
Outer Boundary (the orbital distance at Mars's Equivalent Radiation)
: 0.288 AU ( 43114767.0 km)
Snow Line (the orbital distance at Snow Line Equivalent Radiation)
: 0.424 AU ( 63445268.4 km)
Radiation at Planetary Boundary of SOI-6 b : 0.00 W/m2
(Habitable zone calculated based on SEAU(Solar Equivalent Astronomical Unit) around the star SOI-6)
Kopparapu Recent Venus for Star SOI-6 distance : 0.155 AU
Kopparapu Runaway Greenhouse for Earth-sized planet for Star SOI-6 distance : 0.196 AU
Kopparapu Runaway Greenhouse for Super-Earth-sized planet for Star SOI-6 distance : 0.189 AU
Kopparapu Runaway Greenhouse for Mars-sized planet for Star SOI-6 distance : 0.208 AU
Kopparapu Outer Boundary for Maximum Greenhouse for Star SOI-6 distance : 0.385 AU
Kopparapu Outer Boundary for Early Mars for Star SOI-6 distance : 0.407 AU
(Habitable zone calculated based on Kopparapu et al.(2013) around the star SOI-6)
Original Kopparapu Recent Venus for Star SOI-6 distance : 0.154 AU
Original Kopparapu Runaway Greenhouse for Star SOI-6 distance : 0.203 AU
Original Kopparapu Moist Greenhouse for Star SOI-6 distance : 0.204 AU
Original Kopparapu Outer Boundary for Maximum Greenhouse for Star SOI-6 distance : 0.391 AU
Original Kopparapu Outer Boundary for Early Mars for Star SOI-6 distance : 0.407 AU
(Habitable zone calculated based on Kopparapu et al.(Original) around the star SOI-6)
(Position in Stellar Map of star SOI-6 and its Exoplanet SOI-6 b)
(Zoomed position in Stellar Map of star SOI-6 and its Exoplanet SOI-6 b (zoom level 3))
(Synthetic Spectrum of star SOI-6*)
*Yamashiki YA et al. 2019 ApJ 881 114
MUSCLES Paper I - France et al. 2016 ApJ 820 89
MUSCLES Paper II- Youngblood et al. 2016 ApJ 824 101
MUSCLES Paper III- Loyd et al. 2016 ApJ 824 102