List of unconfirmed exoplanets
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This is a list of unconfirmed extrasolar planets. When a planet candidate is confirmed, please remove it from this list and move it to List of stars with confirmed extrasolar planets.
For a list of unconfirmed brown dwarfs, see list of brown dwarfs.
In addition to known extrasolar planets, there are many planet candidates whose existence is more or less uncertain, or they are now known not to exist.
Contents |
[edit] Probable extrasolar planets
There are a number of exoplanet candidates that are waiting to be confirmed.
star | planet | minimum mass (× Jupiter) |
orbital period (days) |
orbital distance (× Earth) |
orbital eccentricity | inclination | discovery year |
---|---|---|---|---|---|---|---|
1SWASP-J115718.66+261906.1 | b | 1.226804 | 2007 | ||||
1SWASP-J130322.00+350525.4 | b | 2.674207 | 2007 | ||||
1SWASP-J152131.01+213521.3 | b | 1.338018 | 2007 | ||||
1SWASP-J160211.83+281010.4 | b | 3.941554 | 2007 | ||||
1SWASP-J160242.43+290850.1 | b | 1.304693 | 2007 | ||||
1SWASP-J161732.90+242119.0 | b | 1.453738 | 2007 | ||||
unpublished (Anon-1) [1] | 0.3 | 1.3381 | 0.024 | 0 | |||
Beta Pictoris | 2 | 19 y | 8 | ||||
CM Draconis | c | 0.85 | 735 | 1 | |||
COROT-Exo-1 | b | 0.99 | 1.5089557 | 0 | 85.53 | 2007 | |
COROT-Exo-2 | b | 3.53 | 1.7429964 | 0 | 89.13 | 2007 | |
CSI +06-18266 1[2] | |||||||
Epsilon Eridani | c | ~0.1 | ~280 y | ~40 | ~0.3 | 2002 | |
EXP1 J1628-52c07s18161[3] | |||||||
Fomalhaut | 40 | ||||||
GD 66 | b | 2.11 | 1650 | 2.356 | 0 | 2007 | |
Gliese 317 | c | 0.83 | 2700 | 0.42 | 2007 | ||
Gliese 849 | |||||||
GM Aurigae | b | 1.7 | 4 y | 2.5 | |||
HD 111031 | b | 2.87 | 5986 | 0.32 | 2007 | ||
HD 17156 | c | 0.063 | 111.314 | 0.481 | 0.136 | 2008 | |
HD 147506 | c | ||||||
HD 154857 | c | 1900 | 0.25 | 2007 | |||
HD 208487 | c | 0.46? | 908? | 1.8? | 0.19? | ||
HD 24040 | b | 4.04 | 3400 | 4.68 | 0.068 | 2006 | |
HD 28185 | |||||||
HD 50499 | c | 1.7 | 6.8 yr | 2005 | |||
HD 50499 | d | 2 | >10 yr | 2005 | |||
HD 68988 | c | 5.29 | 4100 | 5.32 | 0.01 | 2006 | |
OGLE-TR-111 | c | 0.7 | 16.0644 | 0.12 | |||
OGLE-TR-125 | b | ||||||
OGLE-TR-130 | b | ||||||
OGLE-TR-131 | b | ||||||
OGLE-TR-3 | b | 0.5 | 1.1899 | 0.025 | 90 | ||
Phi2 Pavonis | b | 0.69 | 42.5 | 0.25 | 0.429 | 1998 | |
PSR B1828-11 | b | 0.002 ME | 2007 | ||||
SWEEPS-01 | b | 1.56 | 0.025 | >86 | 2006 | ||
SWEEPS-02 | b | 0.912 | 0.015 | >86 | 2006 | ||
SWEEPS-03 | b | 1.27 | 0.021 | >86 | 2006 | ||
SWEEPS-05 | b | 2.313 | 0.03 | >87 | 2006 | ||
SWEEPS-06 | b | 3.039 | 0.042 | >86 | 2006 | ||
SWEEPS-07 | b | 1.747 | 0.027 | >86 | 2006 | ||
SWEEPS-08 | b | 0.868 | 0.017 | >84 | 2006 | ||
SWEEPS-09 | b | 1.617 | 0.025 | >86 | 2006 | ||
SWEEPS-10 | b | ~1.6 | 0.424 | 0.008 | >84 | 2006 | |
SWEEPS-12 | b | 2.952 | 0.038 | >87 | 2006 | ||
SWEEPS-13 | b | 1.684 | 0.027 | >86 | 2006 | ||
SWEEPS-14 | b | 2.965 | 0.037 | >87 | 2006 | ||
SWEEPS-15 | b | 0.541 | 0.01 | >84 | 2006 | ||
SWEEPS-16 | b | 0.969 | 0.017 | >85 | 2006 | ||
Tau Boötis | |||||||
UNSW-TR 3[4] | |||||||
UNSW-TR 4[5] | |||||||
W 3(OH) | b | 2000 |
[edit] Candidates that cannot be confirmed
Some potential exoplanet candidates have been detected through gravitational microlensing. Since these events are unique and the signal was not clear enough, these planets cannot be confirmed.
star | planet | minimum mass (× Jupiter) |
orbital period (days) |
orbital distance (× Earth) |
discovery year |
---|---|---|---|---|---|
MACHO 94-BLG-4[6] | b | 5 | 1 | 1994 | |
MACHO 95-BLG-3 | b | 2 | 5 | 1995 | |
MACHO 98-BLG-35[7] | b | 1 ME | 1998 | ||
a candidate within the elliptical galaxy YGKOW G1 | 3 ME |
[edit] Doubtful candidates
There are many postulated exoplanets that now seem unlikely to exist.
star | planet | minimum mass (× Jupiter) |
orbital period (days) |
orbital distance (× Earth) |
orbital eccentricity | inclination | discovery year |
---|---|---|---|---|---|---|---|
61 Cygni | Aa | 6 | |||||
Ab | 12 | ||||||
Ba | 7 | ||||||
Aldebaran | b | ~11 | 653.8 | ~2 | 0.182 | 1997 | |
Barnard's Star | b | ||||||
c | |||||||
Geminga | b | 1.7 ME | 5.1 y | 3.3 | 1997 | ||
Gliese 436 | c | 4.7 ME | 5.1859 | 0.0450 | 0.2 | 2008 | |
HD 3346 | b | 10 | 30 | 0.3 | |||
HD 44179 B | b | 1600 | |||||
Iota Horologii | c | 600 | |||||
Lalande 21185 | b | 286.02 | 2118.508 | 2.0 | 0 | ||
c | 508.48 | 10957.8 | 10.0 | 0 | |||
OGLE-2002-BLG-055 | b | 5 | |||||
PSR 0329+54 | A | 0.3 ME | 3.3 y | 2.3 | |||
PSR 0329+54 | B | 2.2 ME | 16.9 y | 7.3 | |||
PSR 1828-10 | A | 3 ME | 0.68 y | 0.93 | |||
PSR 1828-10 | B | 12 ME | 1.35 y | 1.32 | |||
PSR 1828-10 | C | 8 ME | 2.71 y | 2.1 | |||
Upsilon Andromedae A | e | 5 | |||||
Vega | b | 56 |
[edit] Disproven candidates
There are several candidates that have been shown to be more massive than a planet, or not to be real at all.
star | planet | minimum mass (× Jupiter) |
orbital period (days) |
orbital distance (× Earth) |
orbital eccentricity | inclination | discovery year | notes |
---|---|---|---|---|---|---|---|---|
70 Ophiuchi | Ab or Bb | 10 | 17 y | 1855 | ||||
Gliese 570 | b | 0.75 | 400 | 1 | ||||
HD 188753 A | b | 1.14 | 3.3481 | 0.0446 | 0.00 | 2005 | ||
HD 219542 B | b | 0.3 | 112.1 | 0.46 | 0.32 | |||
HD 223084 | b | 1.21 | 104.090 | 0.44 | ||||
HD 34445 | b | 0.58 | 126 | 0.51 | 0.4 | 2004 | ||
HD 83443 | c | 54 ME | 29.83 | 0.174 | 2000 | |||
MACHO-1997-BLG-41 | b | 7 y | 3.5 | |||||
Proxima Centauri | b | 0.666 | ||||||
PSR B1257+12 | D | 100 ME | ~100 y | 40 | 1996 | |||
PSR 1829-10 | 0.5 y | 1991 | ||||||
TMR-1 | C | background star |
[edit] Proplyds with gaps and no known planets
When planets are confirmed, please move to the list of confirmed planets.
Many young stars are accompanied with a protoplanetary disk. Some of the disks have are known to have gaps or other structures which may have been caused by an orbiting planet.
star | gap distance (in AU) |
Notes |
---|---|---|
Beta Pictoris | 50 | Disc is warped |
Cha 110913-773444 | Smallest brown dwarf | |
GM Aurigae | 300 | Disc is warped |
HD 141569 | 86 - 350 | Separates inner and outer regions |
Lynds 1551 | 0.1 | Binary system 45 AU apart |
OTS 44 | Second smallest brown dwarf | |
Vega | 5 | |
Zeta Leporis | 5.4 | First extrasolar protoplanetary disc discovered |
HD 113766 | 1.8, 4-9, 30-80 | Evidence for the formation of Earth-like planets |
HD 98800 B | 5.9 | Spitzer indicated that it may have a planet at between 1.5-2 AU from a star |
[edit] See also
- List of stars with confirmed extrasolar planets
- List of extrasolar planet extremes
- List of hypothetical astronomical objects
- List of stars with proplyds
- List of brown dwarfs
[edit] References
- ^ Notes for star Anon-1
- ^ CSI +06-18266 1 / GSC 00445-01813 SIMBAD
- ^ EXP1 J1628-52c07s18161, SIMBAD essential note
- ^ UNSW-TR 3 SIMBAD
- ^ UNSW-TR 4 SIMBAD
- ^ Planetary Microlensing from the MACHO Project, The MACHO Collaboration 1996
- ^ On Planetary Companions to the MACHO-98-BLG-35 Microlens Star, S.H.Rhie et al. 1999