Article · Wikipedia archive · Last revised Jul 16, 2026

Delta Indi

Delta Indi, Latinized from δ Indi, is a binary star system in the southern constellation of Indus. It is visible to the naked eye with a combined apparent visual magnitude of +4.40. The brighter primary, designated component A, is magnitude 4.80 while the companion, component B, is magnitude 5.96. Based upon an annual parallax shift of 17.34 mas as measured from Earth, the system is located about 188 light years from the Sun.

Last revised
Jul 16, 2026
Read time
≈ 2 min
Length
552 w
Citations
29
Source
Delta Indi
Location of δ Indi (circled in red)
Observation data
Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation Indus
Right ascension 21h 57m 55.07353s1
Declination −54° 59′ 33.2740″1
Apparent magnitude (V) +4.402 (4.80 + 5.96)3
Characteristics
Spectral type F0 IV4
U−B color index +0.102
B−V color index +0.282
Astrometry
Proper motion (μ) RA: +41.941 mas/yr
Dec.: −3.931 mas/yr
Parallax (π)17.34±0.48 mas1
Distance188 ± 5 ly
(58 ± 2 pc)
Absolute magnitude (MV)+0.605
Orbit4
Period (P)12.237±0.080 yr
Semi-major axis (a)0.176±0.004
Eccentricity (e)0.032±0.032
Inclination (i)76.3±2.0°
Longitude of the node (Ω)90.8±2.0°
Periastron epoch (T)2007.518±0.480
Argument of periastron (ω)
(secondary)
64.9±11.0°
Details
δ Ind A
Mass1.78±0.214 M
Luminosity485 L
Surface gravity (log g)3.856 cgs
Temperature7,445±2536 K
Metallicity [Fe/H]−0.215 dex
Rotational velocity (v sin i)1307 km/s
Age4626 Myr
δ Ind B
Mass1.33±0.164 M
Other designations
δ Ind, CPD−55°9733, FK5 824, HD 208450, HIP 108431, HR 8368, SAO 247244, WDS J21579-5500AB8
Database references
SIMBADdata

Delta Indi, Latinized from δ Indi, is a binary star4 system in the southern constellation of Indus. It is visible to the naked eye with a combined apparent visual magnitude of +4.40.2 The brighter primary, designated component A, is magnitude 4.80 while the companion, component B, is magnitude 5.96.3 Based upon an annual parallax shift of 17.34 mas as measured from Earth,1 the system is located about 188 light years from the Sun.

The binary nature of this system was discovered by South African astronomer William Stephen Finsen from 1936 onward,4 with his published orbital elements appearing in 1956.9 The pair have an orbital period of 12.2 years, a semimajor axis of 0.176 arc seconds, and an eccentricity of around 0.03. They have been listed with a stellar classification of F0 IV by multiple authors, suggesting they are yellow-white hued F-type subgiant stars. However, their estimated masses don't match this classification, so Docobo and Andrade (2013) suggest the Hipparcos parallax may have been underestimated.4 One paper has published separate spectral classes of A8(V) and F3(V) respectively for the two components.10

References

References

  1. van Leeuwen, F. (2007), "Validation of the new Hipparcos reduction", Astronomy and Astrophysics, 474 (2): 653–664, arXiv:0708.1752, Bibcode:2007A&A...474..653V, doi:10.1051/0004-6361:20078357, S2CID 18759600.
  2. Nicolet, B. (1978), "Photoelectric photometric Catalogue of homogeneous measurements in the UBV System", Astronomy and Astrophysics Supplement Series, 34: 1–49, Bibcode:1978A&AS...34....1N.
  3. Malkov, O. Yu.; et al. (2012), "Dynamical Masses of a Selected Sample of Orbital Binaries", Astronomy & Astrophysics, 546: 5, Bibcode:2012A&A...546A..69M, doi:10.1051/0004-6361/201219774, A69.
  4. Docobo, J. A.; Andrade, M. (2013), "Dynamical and physical properties of 22 binaries discovered by W. S. Finsen", Monthly Notices of the Royal Astronomical Society, 428 (1): 321–339, Bibcode:2013MNRAS.428..321D, doi:10.1093/mnras/sts045.{{citation}}: CS1 maint: deprecated archival service (link)
  5. Anderson, E.; Francis, Ch. (2012), "XHIP: An extended hipparcos compilation", Astronomy Letters, 38 (5): 331, arXiv:1108.4971, Bibcode:2012AstL...38..331A, doi:10.1134/S1063773712050015, S2CID 119257644.
  6. David, Trevor J.; Hillenbrand, Lynne A. (2015), "The Ages of Early-Type Stars: Strömgren Photometric Methods Calibrated, Validated, Tested, and Applied to Hosts and Prospective Hosts of Directly Imaged Exoplanets", The Astrophysical Journal, 804 (2): 146, arXiv:1501.03154, Bibcode:2015ApJ...804..146D, doi:10.1088/0004-637X/804/2/146, S2CID 33401607.
  7. van Belle, Gerard T. (March 2012), "Interferometric observations of rapidly rotating stars", The Astronomy and Astrophysics Review, 20 (1) 51, arXiv:1204.2572, Bibcode:2012A&ARv..20...51V, doi:10.1007/s00159-012-0051-2, S2CID 119273474.
  8. "del Ind". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2017-08-18.{{cite web}}: CS1 maint: postscript (link)
  9. Finsen, W. S. (1956), "The Orbit of Phi 312 = Delta Indi", Monthly Notes of the Astronomical Society of South Africa, 15: 49, Bibcode:1956MNSSA..15...49F.
  10. Beavers, W. I.; Cook, D. B. (1980), "Scanner studies of composite spectra I. Dwarfs.", The Astrophysical Journal Supplement Series, 44: 489, Bibcode:1980ApJS...44..489B, doi:10.1086/190702.