Epsilon Indi - Revision history

Alastair: add category Stars_with_Planets

2018-05-27T20:52:43Z

add category Stars_with_Planets

Alastair: /* Epsilon Indi */ updates from private wiki - brown dwarfs

2018-05-23T05:32:15Z

Epsilon Indi: updates from private wiki - brown dwarfs

Alastair: Created

2016-10-27T03:58:34Z

Created

New page

== Epsilon Indi ==
=== Fact ===
Epsilon Indi (ε Indi, ε Ind) is a star system approximately 12 light-years from Earth in the constellation of Indus consisting of a K-type main-sequence star, ε Indi A, and two brown dwarfs, ε Indi Ba and ε Indi Bb, in a wide orbit around it. The brown dwarfs were discovered in 2003. ε Indi Ba is an early T dwarf (T1) and ε Indi Bb a late T dwarf (T6) separated by 0.6 arcseconds, with a projected distance of 1460 AU from their primary star.

Estimates provided by the NASA Star and Exoplanet Database indicate that the inner edge of Epsilon Indi's habitable zone could be located around 0.411 AU from the star, while the outer edge edge lies around 0.810 AUs. The distance from the star where an Earth-type planet could have liquid water on its surface is centered around 0.611 AU -- between the orbital distances of Mercury and Venus in our Solar System. At that distance from Epsilon Indi and assuming that it has 0.77 Solar-mass, such a planet would have an orbital period of around 199 days (or a bit over half an Earth year).

The brown dwarfs are likely far enough away from the primary to have negligible effect on any planets in the habitable zone.

[[Image:Artist's Conception of Epsilon Indi System (labelled).jpg|thumb|left|Artist's conception of the Epsilon Indi system showing Epsilon Indi A and its brown-dwarf binary companions.]]

=== Fiction ===
Epsilon Indi is the primary star of the planet [[Taprobane]] (Epsilon Eridani III), home of the [[Timoan]]s.

← Older revision		Revision as of 20:52, 27 May 2018
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		+	[[Category:Stars_with_Planets]]
	== Epsilon Indi ==		== Epsilon Indi ==
	=== Fact ===		=== Fact ===

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 Estimates provided by the NASA Star and Exoplanet Database indicate that the inner edge of Epsilon Indi's habitable zone could be located around 0.411 AU from the star, while the outer edge edge lies around 0.810 AUs. The distance from the star where an Earth-type planet could have liquid water on its surface is centered around 0.611 AU -- between the orbital distances of Mercury and Venus in our Solar System. At that distance from Epsilon Indi and assuming that it has 0.77 Solar-mass, such a planet would have an orbital period of around 199 days (or a bit over half an Earth year).
-The brown dwarfs are likely far enough away from the primary to have negligible effect on any planets in the habitable zone.
+The brown dwarfs are likely far enough away from the primary to have negligible effect on any planets in the habitable zone. Their distance from the star is almost 50 times further than Pluto's average distance from our sun.  (Indeed, our own Solar System could have an undiscovered brown dwarf at that distance.)
 [[Image:Artist's Conception of Epsilon Indi System (labelled).jpg|thumb|left|Artist's conception of the Epsilon Indi system showing Epsilon Indi A and its brown-dwarf binary companions.]]