Observation data Epoch J2000.0 Equinox J2000.0 | |
---|---|
Constellation | Lupus [1] |
Right ascension | 15h 53m 27.29s [2] |
Declination | −42° 16′ 00.7″ [2] |
Apparent magnitude (V) | 7.98 [3] |
Characteristics | |
Spectral type | G2 [3] |
Astrometry | |
Proper motion (μ) | RA: -43.236 mas/yr [2] Dec.: -65.588 mas/yr [2] |
Parallax (π) | 16.6271±0.0221 mas [2] |
Distance | 196.2 ± 0.3 ly (60.14 ± 0.08 pc) |
Other designations | |
NZ Lup, NSV 20423, CD−41 10403, CPD−41 7375, HD 141943, SAO 226339, PPM 321158, TYC 7846-1538-1 [3] | |
Database references | |
SIMBAD | data |
HD 141943 is a young pre-main sequence G-type star with a circumstellar disk. [4] Due to the similarity between HD 141943 and the Sun (Sun-like), it resembles what the Sun would have looked like during the epoch of terrestrial planet formation in Solar System history. [5] Reconstruction of brightness maps of HD 141943 reveal a weak polar spot that changed little in latitude over the 4 year period in which it was observed. It also revealed significant amounts of low latitude features on HD 141943. [6]
It is a potential excellent candidate for telescopes such as the Hubble Space Telescope (HST), the Gemini Planet Imager (GPI) and the Very-Large Telescope (VLT) for follow-up observations of possible planet formation around HD 141943. [7]
The coronal magnetic field of HD 141943 is dominated by a dipole which shows evidence of a possible tilt. The star also has a high differential rotation, about 8 times the value of the magnetic features of the Sun and 5 times the brightness features. This makes it similar to K-type stars. [10]