, there have been no positive confirmations of satellites of extra-solar planets (exomoons); however, some evidence in favour of their existence has been produced.
Host star of the host planet(s) | Planet designation | Planet mass | Planet semimajor axis (AU) | Exomoon semimajor axis | Exomoon mass | Notes | |
---|---|---|---|---|---|---|---|
N/A | J1407b | N/A | 0.396–0.421 AU | <0.8 | One possible exomoon residing in a 4 million km-wide gap in J1407b's circumplanetary disk. Other ring gaps in J1407b's disk may also contain exomoons. | ||
N/A | 2MASS J1119-1137A or B | 3.7 | 3.6 ± 0.9 separation from each other | 0.004 - 0.009 AU | 0.5 - 1 | Found using the transit method. A habitable-zone exomoon candidate transiting a directly imaged free-floating planet or isolated planetary-mass object. | |
N/A | 2MASS J2117-2940 | 7 | N/A | 0.005 AU | ~0.5 | Candidate exomoon transit detected in Spitzer observations of 2MASS J21171431-2940034.[19] | |
10.6 | 330 | 10 AU | 318 | Candidate Jupiter-mass satellite from direct imaging. If confirmed, it could also be considered a planet orbiting a brown dwarf.[20] | |||
1.13 | 0.031 | 0.0087 AU | ? | Found by studying periodic increases and decreases in light given off from HD 189733 b. Outside of planet's Hill sphere.[21] | |||
<0.00112 AU | ~ 0.015 | Exo-Io candidate; The sodium and potassium data[22] [23] at HD 189733b is consistent with evaporating exomoons and/or their corresponding gas torus.[24] | |||||
1.00 | 0.320 | 0.222 RHill | 0.300 | Possible exomoon from transit timing variations, since deemed unlikely. | |||
7.59 | 0.298 | 0.278 RHill | 0.499 | Possible exomoon from transit timing variations, since deemed unlikely. | |||
38.02 | 0.308 | 0.289 RHill | 2.931 | Possible exomoon from transit timing variations. | |||
14.13 | 0.376 | 0.208 RHill | 1.636 | Possible exomoon from transit timing variations. | |||
19.95 | 0.534 | 0.235 RHill | 1.551 | Possible exomoon from transit timing variations, since deemed unlikely. | |||
24.55 | 0.2691 | 0.295 RHill | 6.057 | Possible exomoon from transit timing variations, since deemed unlikely. | |||
14.13 | 0.405 | 0.208 RHill | 1.586 | Possible exomoon from transit timing variations, since deemed unlikely. | |||
[25] | 0.98 | 0.022 AU | 19.0 | Possible Neptune-sized exomoon or double planet, indicated by transit observations.[26] | |||
1.64 | 0.005 AU (11.7 RP) | Possible Neptune-sized exomoon or double planet, indicated by transit observations. | |||||
9.33 | 0.47 | 0.217 RHill | 0.817 | Possible exomoon from transit timing variations, since deemed unlikely. | |||
9.85 | N/A | 0.24 AU | 33.7 | Found by microlensing; however it is unknown if the system is a super-Neptune-mass planet orbiting a free-floating planet, or a binary brown dwarf system.[27] | |||
WASP-12 | WASP-12b[28] | 1.465 | 0.0232 | (radius)[29] | |||
6 RP | Found by studying periodic increases and decreases in light given off from WASP-12b. Outside of planet's Hill sphere. | ||||||
0.37 | 0.0379 | < 1.74 RP | ~ 0.015 | Exo-Io candidate; The sodium exosphere around WASP-49b could be due to a volcanically active Io-like exomoon.[30] | |||
0.92 | 0.033 | 1.125 RP | ~ 0.015 | Exo-Io candidate; Sodium detected via absorption spectroscopy around WASP-76b[31] is consistent with an extrasolar toroidal atmosphere[32] generated by an evaporating exomoon. | |||
1.184 | 0.02544 | ~ 1.9 RP | ~ 0.015 | Exo-Io candidate; The sodium detected via absorption spectroscopy around WASP-121b[33] is consistent with an extrasolar gas torus possibly fueled by a hidden exo-Io. |