Showing posts with label globular. Show all posts
Showing posts with label globular. Show all posts
Friday, 25 August 2017
Globular Cluster NGC 6535
Globular Cluster NGC 6535

This image captures the stunning NGC 6535, a globular cluster 22 000 light-years away in the constellation of Serpens (The Serpent) that measures one light-year across.
Globular clusters are tightly bound groups of stars which orbit galaxies. The large mass in the rich stellar centre of the globular cluster pulls the stars inward to form a ball of stars. The word globulus, from which these clusters take their name, is Latin for small sphere.
Globular clusters are generally very ancient objects formed around the same time as their host galaxy. To date, no new star formations have been observed within a globular cluster, which explains the abundance of aging yellow stars in this image, most of them containing very few heavy elements.
NGC 6535 was first discovered in 1852 by English astronomer John Russell Hind. The cluster would have appeared to Hind as a small, faint smudge through his telescope. Now, over 160 years later, instruments like the Advanced Camera for Surveys (ACS) and Wide Field Camera 3 (WFC3) on the NASA/ESA Hubble Space Telescope allow us to capture the cluster close up and marvel at its contents in detail.
Image Credit: ESA/Hubble & NASA, Gilles Chapdelaine
Explanation from: https://www.spacetelescope.org/images/potw1452a/
download file now
Thursday, 24 August 2017
Globular Cluster NGC 6752
Globular Cluster NGC 6752

Looking like a hoard of gems fit for an emperor�s collection, this deep sky object called NGC 6752 is in fact far more worthy of admiration. It is a globular cluster, and at over 10 billion years old is one the most ancient collections of stars known. It has been blazing for well over twice as long long as our Solar System has existed.
NGC 6752 contains a high number of �blue straggler� stars, some of which are visible in this image. These stars display characteristics of stars younger than their neighbours, despite models suggesting that most of the stars within globular clusters should have formed at approximately the same time. Their origin is therefore something of a mystery.
Studies of NGC 6752 may shed light on this situation. It appears that a very high number � up to 38% � of the stars within its core region are binary systems. Collisions between stars in this turbulent area could produce the blue stragglers that are so prevalent.
Lying 13 000 light-years distant, NGC 6752 is far beyond our reach, yet the clarity of Hubble�s images brings it tantalisingly close.
Image Credit: ESA/Hubble & NASA
Explanation from: https://www.spacetelescope.org/images/potw1205a/
download file now
Subscribe to:
Posts (Atom)