Star Cluster: Difference between revisions
No edit summary |
|||
| Line 7: | Line 7: | ||
[[File:Trumpler_16.png|thumb|TRUMPLER 16]] | [[File:Trumpler_16.png|thumb|TRUMPLER 16]] | ||
Trumpeter 16 is the home of WR 25, currently the most luminous star known in our Milky Way galaxy, together with the less luminous but more massive and famous Eta Carinae star system and the O2 supergiant HD 93129A. | '''Trumpeter 16''' is the home of WR 25, currently the most luminous star known in our Milky Way galaxy, together with the less luminous but more massive and famous '''Eta Carinae''' star system and the O2 supergiant HD 93129A. | ||
Trumpler 16 can be reached by plotting a course to '''CPD-59 2574'''. | '''Trumpler 16''' can be reached by plotting a course to '''CPD-59 2574'''. | ||
'''Eta Carinae''' can be located by name, using the search tool. | |||
==Trumpler 14== | ==Trumpler 14== | ||
[[File:TRUMPLER 14.png|thumb|182x182px|TRUMPLER 14]] | [[File:TRUMPLER 14.png|thumb|182x182px|TRUMPLER 14]] | ||
Trumpler 14 is one of the youngest known star clusters | '''Trumpler 14''' is about half a million years old and one of the youngest known star clusters in the galaxy. Due to its location within the inner parts of the Carina Nebula, Trumpler 14 is currently undergoing massive star formation. As a result, the star cluster exhibits many stars of late '''O''' to early '''A''' spectral type, which are very massive (at least 10 solar masses), short-lived and hot (20000 K). | ||
'''T<span style="font-size:14px;">rumpler 14</span>'''<span style="font-size:14px;"> can be reached by plotting a course to '''CPD-57 3518'''.</span> | |||
A class A blue supergiant can be located near the cluster by plotting a course to '''HD 91969'''. | |||
== Messier 67 == | |||
'''Messier 67''' (also known as M67, NGC 2682, or the Cancri Cluster) is an open cluster in the constellation of Cancer. | |||
[https://www.youtube.com/watch?v=qPDl7158hHQ&feature=youtu.be Distant Stars Expedition] | |||
The cluster had previously been out of reach, due to the 234 light year gap between OUTOTCH SA-U D4-O and AH CANCRI. However, due to a recent discovery of a massive FSD boost via neutron star, what is known as the "Cancri Climb" became possible. However, M67 does not contain any neutron stars. In mid January 2017, a fleet of approximately [https://www.youtube.com/watch?v=JXCOBXG8Px4 360 starships] of the Distant Stars Expedition embarked on a treacherous mission to a system dubbed "Elesium," within the M67 Galaxy... [https://www.youtube.com/watch?v=kEZn7Bdb4iA never to return]. | |||
'''Messier 67''' can be found by searching for '''NGC 2682 FBC 4778'''.[[Category:Stars]] | |||
[[Category:Celestials]] | [[Category:Celestials]] | ||
[[Category:Guides]] | [[Category:Guides]] | ||