Astronomy:Kepler-445

From HandWiki
(Redirected from Astronomy:Kepler-445d)
Short description: Star in the constellation Cygnus
Kepler-445
Observation data
Equinox J2000.0]] (ICRS)
Constellation Cygnus[1]
Right ascension  19h 54m 56.65923s[2]
Declination +46° 29′ 54.7936″[2]
Apparent magnitude (V) 18.19[3]
Characteristics
Evolutionary stage Main sequence
Spectral type M4V[4]
Apparent magnitude (G) 16.685±0.003[2]
Apparent magnitude (J) 13.542±0.029[4]
Apparent magnitude (H) 12.929±0.035[4]
Apparent magnitude (K) 12.610±0.028[4]
Astrometry
Proper motion (μ) RA: 41.465[2] mas/yr
Dec.: 132.351[2] mas/yr
Parallax (π)8.1366 ± 0.0457[2] mas
Distance401 ± 2 ly
(122.9 ± 0.7 pc)
Details[5]
Mass0.334+0.080
−0.059
 M
Radius0.347+0.068
−0.049
 R
Luminosity (bolometric)0.0115 L
Temperature3219+89
−63
 K
Metallicity [Fe/H]+0.27 dex
Other designations
Kepler-445, KOI-2704, KIC 9730163, 2MASS J19545665+4629548[4]
Database references
SIMBADdata

Kepler-445 is a red dwarf star located 401 light-years (123 parsecs) away in the constellation Cygnus. It hosts three known exoplanets, discovered by the transit method using data from the Kepler space telescope and confirmed in 2015.[6] None of the planets orbit within the habitable zone.[7]

Planetary system

Kepler-445b, c, and d orbit Kepler-445 every 3, 5, and 8 days,[3] and have equilibrium temperatures of 401 K (128 °C; 262 °F), 341 K (68 °C; 154 °F), and 305 K (32 °C; 89 °F), respectively.[8] With a radius of 2.72 times that of Earth, Kepler-445c is likely a mini-Neptune with a volatile-rich composition, and has been compared to GJ 1214 b.[6] Kepler-445d is only slightly larger than the Earth, with a radius of 1.33 R.

The Kepler-445 planetary system[5]
Companion
(in order from star)
Mass Semimajor axis
(AU)
Orbital period
(days)
Eccentricity Inclination Radius
b 0.023656 2.98416640+0.00000891
−0.00000936
0.02+0.16
−0.02
89.74+0.18
−0.28
[6]°
1.74+0.29
−0.28
 R
c 0.033427 4.87122714+0.00000636
−0.00000638
0.01+0.16
−0.01
89.91+0.07
−0.10
[6]°
2.72+0.44
−0.43
 R
d 0.047121 8.15272856+0.00006453
−0.00007041
0.01+0.16
−0.01
89.61+0.27
−0.25
[6]°
1.33+0.25
−0.23
 R

References

  1. "Finding the constellation which contains given sky coordinates". 2 August 2008. http://djm.cc/constellation.html. 
  2. 2.0 2.1 2.2 2.3 2.4 Vallenari, A. et al. (2022). "Gaia Data Release 3. Summary of the content and survey properties". Astronomy & Astrophysics. doi:10.1051/0004-6361/202243940  Gaia DR3 record for this source at VizieR.
  3. 3.0 3.1 "Kepler-445". NASA Exoplanet Archive. https://exoplanetarchive.ipac.caltech.edu/overview/Kepler-445. 
  4. 4.0 4.1 4.2 4.3 4.4 "Kepler-445". SIMBAD. Centre de données astronomiques de Strasbourg. http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=Kepler-445. 
  5. 5.0 5.1 Mann, Andrew W.; Dupuy, Trent; Muirhead, Philip S.; Johnson, Marshall C.; Liu, Michael C.; Ansdell, Megan; Dalba, Paul A.; Swift, Jonathan J. et al. (2017), "The Gold Standard: Accurate Stellar and Planetary Parameters for Eight Kepler M Dwarf Systems Enabled by Parallaxes", The Astronomical Journal 153 (6): 267, doi:10.3847/1538-3881/aa7140, Bibcode2017AJ....153..267M 
  6. 6.0 6.1 6.2 6.3 6.4 6.5 Muirhead, Philip S. et al. (March 2015). "Kepler-445, Kepler-446 and the Occurrence of Compact Multiples Orbiting Mid-M Dwarf Stars". The Astrophysical Journal 801 (1): 18. doi:10.1088/0004-637X/801/1/18. Bibcode2015ApJ...801...18M. 
  7. "[...] all of the planets are likely too hot to be located within their host stars’ habitable zones [...]"[6]:8
  8. "Kepler Objects of Interest". http://exoplanetarchive.ipac.caltech.edu/cgi-bin/TblView/nph-tblView?app=ExoTbls&config=cumulative&constraint=koi_pdisposition+like+%27CANDIDATE%27.