Planet NSVS 1425 (AB) b

Detailed information about planet NSVS 1425 (AB) b and its parameters.

Planet

Data Source Type Result Value Result Figure Notes Reference
Molecule Data Source Type Result Value Result Figure Notes Reference

20 Jan 2017 : According to new data by Nasiroglu et al (2017), the planet NSVS 1425 (AB) d replaces the unconfirmed planets NSVS 1425 (AB) b and c. We provisionnaly name it NSVS 1425 (AB) d.
The candidate designated by "c" in Almeida et al. (2012) is designated here as "b", according to the homogeneity convention proposed by Schneider et al; (2012).

19 Feb 2012: A planetary system with the orbital parameter given by Almeida et al. (2012) would be unstable (Wittenmyer et al). More observations are needed.
28 Feb 2012: Beuermann et al. (2012) see a secondary eclipse at phase 0.5002 ± 0.0002.

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Star

Name
NSVS 1425 (AB)
Distance
Spectral type
sdOB+dM
Apparent magnitude V
13.2
Mass
Age
Effective temperature
Radius
Metallicity [Fe/H]
Detected Disc
Magnetic Field
RA2000
20:20:00.0
Dec2000
+04:37:57.0
Alternate Names

Alias 2MASS J20200045+0437564

The parent star is an eclipsing binary with a period of 0.110374 day
The adopted mass is the sum of the two components masses (Almeida et al. 2012)

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