Search results
Results from the WOW.Com Content Network
The Large Magellanic Cloud (LMC) is a dwarf galaxy and satellite galaxy of the Milky Way. [7] At a distance of around 50 kiloparsecs (163,000 light-years), [2] [8] [9] [10] the LMC is the second- or third-closest galaxy to the Milky Way, after the Sagittarius Dwarf Spheroidal (c. 16 kiloparsecs (52,000 light-years) away) and the possible dwarf irregular galaxy called the Canis Major Overdensity.
At the immense distance to the LMC, the parallax method is beyond the limits of current technology. Most estimates assume that R136 is at the same distance as the Large Magellanic Cloud. The most accurate distance to the LMC is 49.97 kpc, derived from a comparison of the angular and linear dimensions of eclipsing binary stars. [3]
SNR 0509-67.5 is a remnant from a supernova in the Large Magellanic Cloud (LMC), that is 160,000 light years away in the constellation Dorado. It displays a clear shock wave shock shell pattern. It was probably a type Ia supernova, as indicated by the detection in 2004 of the elements silicon and iron. Any surviving stars should not have moved ...
A light-year is the distance light travels in a year, 5.9 trillion miles (9.5 trillion km). ... The Large Magellanic Cloud is a satellite galaxy of the Milky Way, as is another nearby galaxy ...
It is a Wolf–Rayet star at the center of R136, the central concentration of stars of the large NGC 2070 open cluster in the Tarantula Nebula (30 Doradus) in the Large Magellanic Cloud. The cluster can be seen in the far southern celestial hemisphere with binoculars or a small telescope, at magnitude 7.25.
Ohnaka’s team used the Very Large Telescope Interferometer to study the star in 2005 and 2007, ... WOH G64 is one of the largest and most luminous stars in the Large Magellanic Cloud, and if it ...
The Large Magellanic Cloud and its neighbour and relative, the Small Magellanic Cloud, are conspicuous objects in the southern hemisphere, looking like separated pieces of the Milky Way to the naked eye. Roughly 21° apart in the night sky, the true distance between them is roughly 75,000 light-years.
It is around 160 to 165 thousand light year distance of the Large Magellanic Cloud and the loose grouping of stars is about 330 to 335 light years across. NGC 2001 is also listed as part of Lucke-Hodge stellar association 64, along with ANONb4 and e135.