Planet CVSO 30 c
| Name | CVSO 30 c | ||
| Planet Status | Controversial | ||
| Discovered in | 2016 | ||
| Mass | 4.7 ( -2.0 +3.6 ) MJ |  |
|
| Mass*sin(i) | — | ||
| Semi-Major Axis | 662.0 (± 96.0) AU | |
+ |
| Orbital Period | — | ||
| Eccentricity | — | ||
| ω | — | ||
| Tperi | — | ||
| Radius | 1.63 ( -0.34 +0.87 ) RJ | |
|
| Inclination | — | ||
| Update | 2017-12-27 | ||
| Detection Method | Imaging | ||
| Mass Detection Method | Spectrum | ||
| Radius Detection Method | Flux | ||
| Primary transit | — | ||
| Secondary transit | — | ||
| λ | — | ||
| Impact Parameter b | — | ||
| Time Vr=0 | — | ||
| Velocity Semiamplitude K | — | ||
| Calculated temperature | — | ||
| Measured temperature | 1600.0 K | |
|
| Hottest point longitude | — | ||
| Geometric albedo | — | ||
| Surface gravity log(g/gH) | — | ||
| Alternate Names | — |
Star
PTFO 8-8695| Name | PTFO 8-8695 | ||
| Distance | 330.0 (± 9.0) pc | |
|
| Spectral type | M3 PMS | ||
| Apparent magnitude V | 16.26 | ||
| Mass | 0.39 (± 0.05) MSun | |
|
| Age | 0.00265 (± 3e-05) Gyr | |
|
| Effective temperature | 3740.0 K | |
|
| Radius | 0.45 (± 0.18) RSun | |
+ |
| Metallicity [Fe/H] | — | ||
| Detected Disc | — | ||
| Magnetic Field | — | ||
| RA2000 | 05:25:08.0 | ||
| Dec2000 | +01:34:24 | ||
| Alternate Names | CVSO 30 | ||
| Planetary system | 1 planet |
Observability Predictor 
Remarks
27 Dec 2017: This planet candidate is claimed to be a background star by Lee and Chiang (2017)18 May 2016: Note that the parent star is designed by CVSO 30 by Schmidt et al. 2016, while it is designed by PTFO 8-8695 by van Eyken et al. 2012
Related publications
Young Exoplanet Transit Initiative follow-up observations of the T Tauri star CVSO 30 with transit-like dips
2022
BISCHOFF R., RAETZ S., FERNANDEZ P., MUGRAUER M., NEIHÄUSER R. et al.
MNRAS, 511, 3497
paper
Color Dependence of Planetary Transit Depths due to Large Starspots and Dust Clouds: Application to PTFO 8-8695
2021
GROSSON Th. & JOHNS-KRULL Ch.
Res. Notes AAS., 5, 264
paper
Properties of CVSO 30 from TESS measurements: probably a binary T Tauri star with complex light curves and no obvious planets
2020
KOEN C.
MNRAS, 494, 4349
paper
PTFO 8-8695: Two Stars, Two Signals, No Planet
2020
BOUMA L., WINN J., RICKER G., VANDERSPEK R., LATHAM D. et al.
Astron. J., 160, 86
paper arxiv
Evidence for planetary hypothesis for PTFO 8-8695b with five-year optical/infrared monitoring observations
2020
TANIMOTO Y., YAMASHITA T., UI T., UCHIYAMA M., KAWABATA M. et al.
PASJ, accepted
arxiv
Evidence that the planetary candidate CVSO30c is a background star from optical, seeing-limited data
2018
LEE Ch.-H., CHIANG P.-Sh.
ApJ Lett, 852, L24
paper arxiv
Multi-Color Simultaneous Photometry of the T-Tauri Star Having A Planetary Candidate CVSO 30
2017
ONITSUKA M., FUKUI A.,NARITA N., HIRANO T., KUSAKABE N. et al.
PASJ, 69, L2
arxiv
paper
Direct Imaging discovery of a second planet candidate around the possibly transiting planet host CVSO 30
2016
SCHMIDT T., NEUHÄUSER R., BRICEÑO C., VOGT N., RAETZ S. et al.
Astron. & Astrophys., accepted
arxiv
The PTF Orion Project: a Possible Planet Transiting a T-Tauri Star
2012
van EYKEN J., CIARDI D., von BRAUN K., KANE S., PLAVCHAN P. & 32 addiional authors
ApJ., 755, 42
paper arxiv
arxiv
