Planet 1SWASP J1407 b
| Name | 1SWASP J1407 b | ||
| Planet Status | Confirmed | ||
| Discovered in | 2012 | ||
| Mass | — | ||
| Mass*sin(i) | 20.0 ( -6.0 +6.0 ) MJ |  |
|
| Semi-Major Axis | 3.9 (± 1.7) AU | |
|
| Orbital Period | 3725.0 (± 900.0) day | |
|
| Eccentricity | — | ||
| ω | — | ||
| Tperi | — | ||
| Radius | — | ||
| Inclination | — | ||
| Update | 2014-10-29 | ||
| Detection Method | Primary Transit | ||
| Mass Detection Method | Radial Velocity | ||
| Radius Detection Method | — | ||
| Primary transit | — | ||
| Secondary transit | — | ||
| λ | — | ||
| Impact Parameter b | — | ||
| Time Vr=0 | — | ||
| Velocity Semiamplitude K | — | ||
| Calculated temperature | — | ||
| Measured temperature | — | ||
| Hottest point longitude | — | ||
| Geometric albedo | — | ||
| Surface gravity log(g/gH) | — | ||
| Alternate Names | — |
Star
1SWASP J1407| Name | 1SWASP J1407 | ||
| Distance | 133.0 (± 12.0) pc | |
|
| Spectral type | |||
| Apparent magnitude V | 12.4 | ||
| Mass | 0.9 MSun | |
|
| Age | 0.016 Gyr | |
|
| Effective temperature | 4400.0 (± 100.0) K | |
|
| Radius | 0.99 (± 0.11) RSun | ||
| Metallicity [Fe/H] | — | ||
| Detected Disc | — | ||
| Magnetic Field | — | ||
| RA2000 | 14:07:48.0 | ||
| Dec2000 | -39:45:43 | ||
| Alternate Names | |||
| Planetary system | 1 planet |
Observability Predictor 
Remarks
29 Oct 2014: The object J1407 b is surrounded by a ring-like structure (Mamajek et al. 2012, Kenworthy et al. 2014)Related publications
A Self-Gravitating Exoring Around J1407b and Implications for In-Situ Exomoon Formation
2022
SUTTON Ph., ALBERY B. & MUFF J.
Front. Astron. Space Sci.,, 9, in press
paper
Scattered light may reveal the existence of ringed exoplanets
2020
SUCERQUIA M., LAVARADO-MONTES J., ZULUEGA J., MONESINOS M. & BAYO A.
MNRAS, 496, L85
paper arxiv
ALMA and NACO observations towards the young exoring transit system J1407 (V1400 Cen)
2019
KENWORTHY M., KLAASSEN P., MIN M., van der MAREL N., BOHN A. et al.
Astron. & Astrophys., 633, A115
paper arxiv
Mean Motion Resonances With Nearby Moons: An Unlikely Origin For The Gaps Observed In The Ring Around The Exoplanet J1407b
2019
SUTTON Ph.
MNRAS, 486, 1681
paper arxiv
Constraining the period of the ringed secondary companion to the young star J1407 with photographic plates
2018
MENTEL R., KENWORTHY M., CAMERON D., SCOTT E., MELLON S. et al.
Astron. & Astrophys., 619, A157
paper arxiv
Exploration of the brown dwarf regime around solar-like stars by CoRoT
2016
CSIZMADIA Sz.
in "'The CoroT legacy book", 2016, Editors: Annie Baglin et al., Publisher: EDP Sciences
arxiv
Modeling giant extrasolar ring systems in eclipse and the case of J1407b: sculpting by exomoons?
2015
KENWORTHY M. & MAMAJEK E.
ApJ, 800, 126
paper ADS arxiv
Mass and period limits on the ringed companion transiting the young star J1407
2014
KENWORTHY M., LACOUR S., KRAUS A., TRIAUD A., MAMAJEK E. et al.
MNRAS, 446, 411
paper arxiv
Planetary Construction Zones in Occultation: Discovery of an Extrasolar Ring System Transiting a Young Sun-like Star and Future Prospects for Detecting Eclipses by Circumsecondary and Circumplanetary Disks
2012
MAMAJEK E., QUILLEN A., PECAUT M., MOOLEKAMP F., SCOTT E. & 3 additional authors
Astron. J., 143, 72
paper arxiv
