Jump to content
Main menu
Main menu
move to sidebar
hide
Navigation
Main page
Recent changes
Random page
Help about MediaWiki
Special pages
Niidae Wiki
Search
Search
Appearance
Create account
Log in
Personal tools
Create account
Log in
Pages for logged out editors
learn more
Contributions
Talk
Editing
Sextans
(section)
Page
Discussion
English
Read
Edit
View history
Tools
Tools
move to sidebar
hide
Actions
Read
Edit
View history
General
What links here
Related changes
Page information
Appearance
move to sidebar
hide
Warning:
You are not logged in. Your IP address will be publicly visible if you make any edits. If you
log in
or
create an account
, your edits will be attributed to your username, along with other benefits.
Anti-spam check. Do
not
fill this in!
=== Multiple star systems === Sextans contains a few notable multiple star systems within its boundaries. [[35 Sextantis]] is a triple star system consisting of two evolved [[K-type giant]]s of equal mass, with both stars being twice as massive as the Sun.<ref name = Tokovinin2008>{{cite journal | last=Tokovinin | first=A. | title=Comparative statistics and origin of triple and quadruple stars | journal=Monthly Notices of the Royal Astronomical Society | volume=389 | issue=2 | date= September 11, 2008 | doi=10.1111/j.1365-2966.2008.13613.x | pages=925β938 | bibcode = 2008MNRAS.389..925T | arxiv = 0806.3263 | doi-access = free}}</ref> The secondary is itself a single-lined [[spectroscopic binary]] consisting of a {{solar mass|0.58|link=y}} companion and itself.<ref name = Tokovinin2008/> The system is located approximately 700 light years away.<ref name = GaiaDR3A>{{Cite DR3|3858258736489909632}}</ref><ref name = GaiaDR3B>{{Cite DR3|3858258736489910400}}</ref> The outer pair has a separation of 6.8" and both stars take roughly 23,000 years to orbit each other while the B subsystem takes 1,528 days to circle each other in a relatively [[orbital eccentricity|eccentric]] orbit.<ref name = Tokovinin2007>{{cite journal | last=Tokovinin | first=A. A. | last2=Gorynya | first2=N. A. | title=New spectroscopic components in multiple systems. V. | journal=Astronomy & Astrophysics | volume=465 | issue=1 | date = April 2007 | issn=0004-6361 | doi=10.1051/0004-6361:20066888 | s2cid = 34100030 | pages=257β261 | bibcode = 2007A&A...465..257T | doi-access = free}}</ref> There are a few notable [[variable star]]s, including [[25 Sextantis|25]], [[23 Sextantis]], and [[LHS 292]]. [[NGC 3115]], an edge-on [[lenticular galaxy]], is the only noteworthy [[deep-sky object]]. It also lies near the ecliptic, which causes the [[Moon]], and some of the planets to occasionally pass through it for brief periods of time. The constellation is the location of the field studied by the [[Cosmic Evolution Survey|COSMOS project]], undertaken by the [[Hubble Space Telescope]].
Summary:
Please note that all contributions to Niidae Wiki may be edited, altered, or removed by other contributors. If you do not want your writing to be edited mercilessly, then do not submit it here.
You are also promising us that you wrote this yourself, or copied it from a public domain or similar free resource (see
Encyclopedia:Copyrights
for details).
Do not submit copyrighted work without permission!
Cancel
Editing help
(opens in new window)
Search
Search
Editing
Sextans
(section)
Add topic