| Observation data Epoch J2000.0 Equinox J2000.0 | |
|---|---|
| Constellation | Serpens |
| Right ascension | 15h 45m 39.0752s [1] |
| Declination | +14° 22′ 31.7590″ [1] |
| Apparent magnitude (V) | ~5 Max. 16.6 Min. [2] |
| Characteristics | |
| Spectral type | CV [3] |
| Variable type | Nova [2] |
| Astrometry | |
| Proper motion (μ) | RA: 3.780±0.119 [1] mas/yr [1] Dec.: −22.338±0.095 mas/yr [1] |
| Parallax (π) | 0.2304±0.0629 mas [1] |
| Distance | 2774+495 −268 [2] pc |
| Details | |
| Surface gravity (log g) | 9.88±0.13 [3] cgs |
| Temperature | 10,772±230 [3] K |
| Other designations | |
| Nova Ser 1948, AAVSO 1541+14, 2MASS J15453907+1422317 [4] | |
| Database references | |
| SIMBAD | data |
CT Serpentis (also known as Nova Serpentis 1948) was a nova that appeared in the constellation Serpens in 1948. It was discovered by Ramze Alexander Bartaya at Abastumani Observatory on 9 April 1946. [5] [6] It is thought to have reached magnitude 6.0, [7] but this is an extrapolation of its light curve as it was not observed until 9 April 1948 when it was at magnitude 9.0 and fading—clearly past its maximum. [8]