Planet KOI-2700 b

Name KOI-2700 b
Planet Status Confirmed
Discovered in 2013
Mass 0.00271 ( -0.00271 +0.0 ) MJ
Mass*sin(i)
Semi-Major Axis
Orbital Period 0.910022 (± 5e-06) day
Eccentricity
ω
Tperi
Radius 0.0946 ( -0.0946 +0.0 ) RJ
Inclination
Update 2018-11-20
Detection Method Primary Transit
Mass Detection Method
Radius Detection Method
Primary transit 2454900.358 (± 0.004) JD
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

KOI-2700
Name KOI-2700
Distance
Spectral type
Apparent magnitude V 15.9
Mass 0.632 (± 0.063) MSun
Age
Effective temperature 4433.0 (± 66.0) K
Radius 0.574 (± 0.05) RSun
Metallicity [Fe/H] -0.2
Detected Disc
Magnetic Field
RA2000 19:48:01.0
Dec2000 +44:46:30
Alternate Names
Planetary system 1 planet

More data

Observability Predictor

Remarks

11 Dec 2013: The transit light curve is very asymmetric, suggesting the presence of a cometary like dust tail. Therefore the planet radius itself and the inferred mass are hard to estimate (Rappaport et al. 2013).

Related publications

Light-curve analysis of KOI 2700b: the second extrasolar planet with a comet-like tail
2017 GARAI Z.
Astron. & Astrophys., accepted
arxiv  

KOI-2700b - A Planet Candidate With Dusty Effluents on a 22-Hour Orbit
2014 RAPPAPORT S., BARCLAY T., DEVORE J., ROWE J., SANCHIS-OJEDA R. & STILL M.
ApJ, 784, 40
paper  arxiv  

Dusty tails of evaporating exoplanets. I. Constraints on the dust composition
2014 van LIESHOUT R., MIN M. & DOMINIK C.
Astron. & Astrophys., 572, A76
paper  arxiv