Credit & Copyright: Xinran Li
Explanation:
Why are there so many bright blue stars?
Stars are usually born in clusters, and the brightest and
most massive of these stars typically glow blue.
Less-bright, non-blue stars like our
Sun
surely also exist in this
M41 star cluster but are harder to see.
A few bright orange-appearing
red giant stars are visible.
The red-light filaments are emitted by diffuse hydrogen gas, a
color that was specifically filtered and enhanced in this image.
In a hundred million years or so, the bright blue stars will have exploded in
supernovas and disappeared,
while the slightly different trajectories of the fainter stars will cause
this picturesque open cluster to disperse.
Similarly, billions of years ago, our own Sun was likely born into a
star cluster
like M41, but it has long since
drifted
apart from its
sister stars.
The featured image was captured over four hours with
Chilescope T2 in
Chile.
1999 2000 2001 2002 2003 2004 2005 2006 2007 2008 2009 2010 2011 2012 2013 2014 2015 2016 2017 2018 2019 2020 2021 2022 2023 2024 2025 |
Январь Февраль Март Апрель Май Июнь Июль Август Сентябрь Октябрь Ноябрь Декабрь |
NASA Web Site Statements, Warnings, and Disclaimers
NASA Official: Jay Norris. Specific rights apply.
A service of: LHEA at NASA / GSFC
& Michigan Tech. U.
|
Публикации с ключевыми словами:
open cluster - Рассеянное скопление
Публикации со словами: open cluster - Рассеянное скопление | |
См. также:
Все публикации на ту же тему >> | |
