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NGTS-3

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Binary star in the constellation Columba.
NGTS-3
Observation data
Epoch J2000      Equinox J2000
Constellation Columba
Right ascension 06 17 46.75
Declination −35° 42′ 23.05″
Apparent magnitude (V) 14.67±0.01
Characteristics
Spectral type G6 V + K1 V
B−V color index +0.77
R−I color index +0.36
Astrometry
Radial velocity (Rv)8.57±0.05 km/s
Proper motion (μ) RA: -8.838 mas/yr
Dec.: +8.771 mas/yr
Parallax (π)1.3153 ± 0.0193 mas
Distance2,480 ± 40 ly
(760 ± 10 pc)
Details
A
Mass1.02±0.09 M
Radius0.93±0.23 R
Luminosity0.72±0.03 L
Surface gravity (log g)4.45 cgs
Temperature5,600±150 K
Metallicity 0.12±0.15 dex
Rotational velocity (v sin i)1.0±0.7 km/s
Other designations
Gaia DR2 2885350546895266432
Database references
SIMBADdata
Exoplanet Archivedata

NGTS-3 is a star system located in the southern constellation Columba. With an apparent magnitude of 14.67, it requires a powerful telescope to observe. However, NGTS-3 is actually an unresolved spectroscopic binary system. The system is located approximately 2,480 light years away, based on parallax measurement, and is receding with a radial velocity of 8.57 km/s.

The system consists of two main sequence stars, classified as G6 and K1, respectively; however, only the properties of the primary star are known. NGTS-3A has a similar mass to that of the Sun, but is 7% smaller in radius. It radiates at 72% of the Sun's luminosity from its photosphere at an effective temperature of 5,600 K, which gives it the typical yellow hue characteristic of a G-type star.

Planetary System

In 2018, the NGTS survey discovered an inflated hot Jupiter orbiting NGTS-3A despite the components being visually unresolved.

The NGTS-3A planetary system
Companion
(in order from star)
Mass Semimajor axis
(AU)
Orbital period
(days)
Eccentricity Inclination Radius
b 2.38 ± 0.26 MJ 0.023+0.007
−0.005
1.6753728 ± 0.0000030 0? 89.56+0.31
−0.48°
1.48 ± 0.37 RJ

References

  1. ^ Brown, A. G. A.; et al. (Gaia collaboration) (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties". Astronomy & Astrophysics. 616. A1. arXiv:1804.09365. Bibcode:2018A&A...616A...1G. doi:10.1051/0004-6361/201833051. Gaia DR2 record for this source at VizieR.
  2. ^ Zacharias, N.; Finch, C. T.; Girard, T. M.; Henden, A.; Bartlett, J. L.; Monet, D. G.; Zacharias, M. I. (February 2013). "The Fourth US Naval Observatory CCD Astrograph Catalog (UCAC4)". The Astronomical Journal. 145 (2): 44. arXiv:1212.6182. Bibcode:2013AJ....145...44Z. doi:10.1088/0004-6256/145/2/44. ISSN 0004-6256. S2CID 119299381.
  3. ^ Günther, Maximilian N.; et al. (August 2018). "Unmasking the hidden NGTS-3Ab: a hot Jupiter in an unresolved binary system". Monthly Notices of the Royal Astronomical Society. 478 (4): 4720–4737. arXiv:1805.01378. Bibcode:2018MNRAS.478.4720G. doi:10.1093/mnras/sty1193. ISSN 0035-8711.
  4. Stassun, Keivan G.; et al. (October 2019). "The Revised TESS Input Catalog and Candidate Target List". The Astronomical Journal. 158 (4): 138. Bibcode:2019AJ....158..138S. doi:10.3847/1538-3881/ab3467. hdl:1721.1/124721. ISSN 0004-6256. S2CID 166227927.
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