NSVS 14256825
Observation data J2000
| ||
---|---|---|
Constellation | Aquila | |
Right ascension | 20h 20m 00.45867s[2] | |
Declination | +04° 37′ 56.5198″[2] | |
Apparent magnitude (V) | 13.2[3] | |
Characteristics | ||
Spectral type | sdOB / M V[3] | |
Periastron epoch (T) | 2454274.20874 JD | |
Details[3] | ||
Mass | 0.528 M☉ | |
Temperature | 42,000 K | |
Database references | ||
SIMBAD | data |
NSVS 14256825, also known as V1828 Aquilae, is an
Nomenclature
The system is most commonly referred to using its designation from the Northern Sky Variability Survey (NSVS), a survey of stars with
Eclipse timing variations
NSVS 14256825 has been extremely well-studied using
Initially, in 2012 it was claimed that two giant planets were in orbit around the binary, with masses of 2.9 and 8.1 times the mass of Jupiter orbiting with periods of 3.5 and 6.9 years respectively.[1] Another paper claimed the existence of one planet with a mass 12 times that of Jupiter, in a 20-year orbit.[11] However, subsequent studies have come up with different results with masses up to 15 MJ[9] and periods down to 8.83 years.[12] Studies also do not agree on whether one substellar body can explain the ETVs, or whether additional companions are necessary, but further research is needed to obtain better coverage of data.[13]
See also
- HW Virginis
- CM Draconis
- QS Virginis
- NN Serpentis
- List of extrasolar planets
References
- ^ S2CID 119177743.
- ^ .
- ^ a b c "Notes on NSVS 1425 (AB) b". Extrasolar Planets Encyclopaedia. Retrieved 26 November 2016.
- S2CID 53724563.
- ^ a b "NSVS 14256825". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2020-10-16.
- S2CID 2974543.
- ^ S2CID 54997940.
- .
- ^ S2CID 118936443.
- hdl:10566/891.
- S2CID 119267859.
- S2CID 135471537.
- S2CID 231662494.