Hubble ACS/HRC image showing all three stars. Upper left is LTT 1445 A and in the lower right part of the image is the LTT 1445 BC pair. | |
Observation data Epoch J2000.0 Equinox J2000.0 | |
---|---|
Constellation | Eridanus |
LTT 1445 A | |
Right ascension | 03h 01m 51.39367s[1] |
Declination | −16° 35′ 36.0312″[1] |
Apparent magnitude (V) | 11.22±0.02[2] |
LTT 1445 BC | |
Right ascension | 03h 01m 51.04s[2] |
Declination | −16° 35′ 31.1″[2] |
Apparent magnitude (V) | 11.37±0.03[2] |
Characteristics | |
Spectral type | M2.5+M3.0+M[3][2] |
Astrometry | |
LTT 1445 A | |
Radial velocity (Rv) | −5.74±0.33[1] km/s |
Proper motion (μ) | RA: −369.972 mas/yr[1] Dec.: −267.931 mas/yr[1] |
Parallax (π) | 145.6922 ± 0.0244 mas[1] |
Distance | 22.387 ± 0.004 ly (6.864 ± 0.001 pc) |
Orbit[2] | |
Primary | LTT 1445 B |
Companion | LTT 1445 C |
Period (P) | 36.2±5.3 yr |
Semi-major axis (a) | 1.159±0.076″ |
Eccentricity (e) | 0.50±0.11 |
Inclination (i) | 89.64±0.13° |
Longitude of the node (Ω) | 137.63±0.19° |
Periastron epoch (T) | 2019.2±1.7 |
Argument of periastron (ω) (secondary) | 209±13° |
Details | |
A | |
Mass | 0.257±0.014 M☉[4] M☉ |
Radius | 0.271+0.019 −0.010 R☉[4] R☉ |
Luminosity (bolometric) | 0.00805±0.00035[2] L☉ |
Surface gravity (log g) | 4.967+0.061 −0.075[2] cgs |
Temperature | 3,337±150[2] K |
Metallicity [Fe/H] | −0.34±0.08[2] dex |
B | |
Mass | 0.215±0.014[2] M☉ |
Radius | 0.236±0.027[2] R☉ |
C | |
Mass | 0.161±0.014[2] M☉ |
Radius | 0.197±0.027[2] R☉ |
Rotation | 1.4 d[4] |
Other designations | |
Database references | |
SIMBAD | A,BC |
LTT 1445 is a triple M-dwarf system 22.4 light-years (6.9 parsecs) distant[1] in the constellation Eridanus. The primary LTT 1445 A hosts two exoplanets—one discovered in 2019 that transits the star every 5.36 days, and another found in 2021 that transits the star every 3.12 days, close to a 12:7 resonance. As of October 2022 it is the second closest transiting exoplanet system discovered, with the closest being HD 219134 bc.[5]
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