Magnitude +10.4 globular cluster NGC 1854 (α=05h 09m 20.2s, δ=-68° 50′ 56″ J2000.0) was discovered in 1826 by James Dunlop. It lies 135,000 light-years away in the Large Magellanic Cloud. This Hubble Space Telescope view is just 2.4 x 1.5 arcminutes in size. Click the image for a larger version. Image credit: ESA/Hubble & NASA.This NASA/ESA Hubble Space Telescope image shows the globular cluster NGC 1854, a gathering of white and blue stars in the southern constellation of Dorado (The Dolphinfish). NGC 1854 is located about 135,000 light-years away, in the Large Magellanic Cloud (LMC), one of our closest cosmic neighbours and a satellite galaxy of the Milky Way.
The LMC is a hotbed of vigorous star formation. Rich in interstellar gas and dust, the galaxy is home to approximately 60 globular clusters and 700 open clusters. These clusters are frequently the subject of astronomical research, as the Large Magellanic Cloud and its little sister, the Small Magellanic Cloud, are the only systems known to contain clusters at all stages of evolution. Hubble is often used to study these clusters as its extremely high-resolution cameras can resolve individual stars, even at the clusters’ crowded cores, revealing their mass, size and degree of evolution.
Scientists from Rosetta’s OSIRIS team have discovered an extraordinary formation in the Aker region on the larger lobe of comet 67P/Churyumov-Gerasimenko. The largest of a group of three boulders with a diameter of approximately 30 metres appears to perch on the rim of a small depression. There seems to be only a very small contact area with the nucleus.
This infrared image from ESA’s Herschel Space Observatory shows the region known as Vulpecula OB1, a ‘stellar association’ in which a batch of truly giant ‘OB’ stars is being born 8,000 light-years away in the constellation of Vulpecula (The Little Fox). There is enough material here to build stars for millions of years to come.
