To install click the Add extension button. That's it.

The source code for the WIKI 2 extension is being checked by specialists of the Mozilla Foundation, Google, and Apple. You could also do it yourself at any point in time.

4,5
Kelly Slayton
Congratulations on this excellent venture… what a great idea!
Alexander Grigorievskiy
I use WIKI 2 every day and almost forgot how the original Wikipedia looks like.
Live Statistics
English Articles
Improved in 24 Hours
Added in 24 Hours
What we do. Every page goes through several hundred of perfecting techniques; in live mode. Quite the same Wikipedia. Just better.
.
Leo
Newton
Brights
Milds

From Wikipedia, the free encyclopedia

η Indi
Location of η Indi (circled)
Observation data
Epoch J2000      Equinox J2000
Constellation Indus
Right ascension 20h 44m 02.33404s[1]
Declination −51° 55′ 15.4970″[1]
Apparent magnitude (V) 4.52[2]
Characteristics
Spectral type A9IV[3]
B−V color index +0.26[2]
Astrometry
Radial velocity (Rv)−1.6±0.8[4] km/s
Proper motion (μ) RA: +155.80[1] mas/yr
Dec.: −53.86[1] mas/yr
Parallax (π)41.37 ± 0.25 mas[1]
Distance78.8 ± 0.5 ly
(24.2 ± 0.1 pc)
Absolute magnitude (MV)2.59[5]
Details
Mass1.60[6] M
Radius2.27[7] R
Luminosity7.60[5] L
Temperature7,694[6] K
Rotational velocity (v sin i)75[8] km/s
Age100±50[7] Myr
Other designations
η Ind, CPD−52° 11752, FK5 776, HD 197157, HIP 102333, HR 7920, SAO 246709[2]
Database references
SIMBADdata

Eta Indi, Latinised from η Indi, is a single, white-hued star in the southern constellation Indus. It is a faint star but visible to the naked eye with an apparent visual magnitude of 4.52.[2]

Measurements with the Hipparcos spacecraft showed the star, which is single,[9] appears to move against the deep sky backdrop by a mean biannual parallax shift of around 41.37 mas,[1] which equates to 79 light-years' distance. Its radial vector to our system's own trajectory (radial velocity) shows it to be in a phase of a narrowing of the gap, at a rounded −2 km/s, net.[4] η Indi appears to be a member of the Octans association, a group of 62 stars that are around 30−50 million years old and have common motion.[10]

The spectrum of this star matches a stellar classification of A9 IV[3] which suggests it is an evolving subgiant star of type A. The star is estimated 1.6 M (masses of the Sun),[6] and 2.27 R (its radius).[7] It is shines with 7.60[5] times the Sun's luminosity, which is radiated from its photosphere at an effective temperature of 7,694 K.[6] The star is spinning with a projected rotational velocity of 75 km/s.[8] It is very likely to be a hybrid Delta Scuti/Gamma Doradus variable.[8]

References

  1. ^ a b c d e f 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. Vizier catalog entry
  2. ^ a b c d "Eta Indi". SIMBAD Astronomical Database. Retrieved 2016-08-23.
  3. ^ a b Gray, R. O.; et al. (July 2006). "Contributions to the Nearby Stars (NStars) Project: spectroscopy of stars earlier than M0 within 40 pc-The Southern Sample". The Astronomical Journal. 132 (1): 161–170. arXiv:astro-ph/0603770. Bibcode:2006AJ....132..161G. doi:10.1086/504637. S2CID 119476992.
  4. ^ a b Gontcharov, G. A. (November 2006). "Pulkovo Compilation of Radial Velocities for 35 495 Hipparcos stars in a common system". Astronomy Letters. 32 (11): 759–771. arXiv:1606.08053. Bibcode:2006AstL...32..759G. doi:10.1134/S1063773706110065. S2CID 119231169.
  5. ^ a b c Anderson, E.; Francis, Ch. (May 2012). "XHIP: An extended hipparcos compilation". Astronomy Letters. 38 (5): 331–346. arXiv:1108.4971. Bibcode:2012AstL...38..331A. doi:10.1134/S1063773712050015. S2CID 119257644. Vizier catalog entry
  6. ^ a b c d David, Trevor J.; Hillenbrand, Lynne A. (May 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): 146–184. arXiv:1501.03154. Bibcode:2015ApJ...804..146D. doi:10.1088/0004-637X/804/2/146. S2CID 33401607. Vizier catalog entry
  7. ^ a b c Plavchan, Peter; et al. (June 2009), "New Debris Disks Around Young, Low-Mass Stars Discovered with the Spitzer Space Telescope", The Astrophysical Journal, 698 (2): 1068–1094, arXiv:0904.0819, Bibcode:2009ApJ...698.1068P, doi:10.1088/0004-637X/698/2/1068, S2CID 51417657.
  8. ^ a b c Koen, C.; van, Wyk F.; Laney, C. D.; Kilkenny, D. (2017), "HR 7920: a very bright new Delta Scuti star with possible Gamma Doradus variations", MNRAS, 466 (1): 122–128, Bibcode:2017MNRAS.466..122K, doi:10.1093/mnras/stw3062
  9. ^ Rodriguez, David R.; et al. (May 2015), "Stellar multiplicity and debris discs: an unbiased sample", Monthly Notices of the Royal Astronomical Society, 449 (3): 3160–3170, arXiv:1503.01320, Bibcode:2015MNRAS.449.3160R, doi:10.1093/mnras/stv483.
  10. ^ Torres, C. A. O.; Quast, G. R.; da Silva, L .; de la Reza, R.; Melo, C. H. F.; Sterzik, M. (2006). "Search for associations containing young stars (SACY)". Astronomy and Astrophysics. 460 (3): 695–708. arXiv:astro-ph/0609258. Bibcode:2006A&A...460..695T. doi:10.1051/0004-6361:20065602. ISSN 0004-6361. S2CID 16080025.
This page was last edited on 27 March 2022, at 06:49
Basis of this page is in Wikipedia. Text is available under the CC BY-SA 3.0 Unported License. Non-text media are available under their specified licenses. Wikipedia® is a registered trademark of the Wikimedia Foundation, Inc. WIKI 2 is an independent company and has no affiliation with Wikimedia Foundation.