This is a zoomed-in section of the 46 billion-pixel Milky Way picture depicting the Eta Carinae Nebula. An online tool provided by astronomers at the Ruhr-Universität Bochum (RUB) permits users to navigate the huge image by named object or celestial coordinates, zoom in or out, or apply specific filters. Image credit: Lehrstuhl für Astrophysik, RUB. AN screen capture by Ade Ashford.For five years, the astronomers at the Ruhr-Universität Bochum (RUB) have been monitoring our galaxy in the search of objects with variable brightness. Those objects may, for example, include stars in front of which a planet is passing, or multiple systems where stars orbit each other and which obscure each other every now and then. In his PhD thesis, Moritz Hackstein is compiling a catalogue of such variable objects of medium brightness. For this purpose, the team from the Faculty of Physics and Astronomy takes pictures of the southern sky night after night. To this end, they use the telescopes at Bochum’s university observatory in the Atacama Desert in Chile. More than 50,000 new variable objects, which had hitherto not been recorded in databanks, have been discovered by the researchers so far.
268 Individual Images Make Up the Photo of the Milky Way
The area that the astronomers observe is so large that they have to subdivide it into 268 sections. They photograph each section in intervals of several days. By comparing the images, they are able to identify the variable objects. The team has assembled the individual images of the 268 sections into one comprehensive image. Following a calculation period of several weeks, they created a 194 Gigabyte file, into which images taken with different filters have been entered.
Online Tool Facilitates Search for Individual Celestial Objects
Using the online tool, any interested person can view the complete ribbon of the Milky Way at a glance, or zoom in and inspect specific areas. An input window, which provides the position of the displayed image section, can be used to search for specific objects. If the user types in “Eta Carinae,” for example, the tool moves to the respective star; the search term “M8” leads to the Lagoon Nebula.
This NASA/ESA Hubble Space Telescope image captures the remnants of a long-dead star. These rippling wisps of ionised gas, named DEM L316A, are the remains of an especially energetic Type Ia supernova located some 160,000 light-years away within one of the Milky Way’s closest galactic neighbours — the Large Magellanic Cloud (LMC).
Just in time for the release of the movie “Star Wars Episode VII: The Force Awakens,” NASA’s Hubble Space Telescope has photographed what looks like a cosmic, double-bladed lightsabre. In the centre of the image, partially obscured by a dark, Jedi-like cloak of dust, a newborn star shoots twin jets out into space as a sort of birth announcement to the universe.
Planetary nebulae such as Hen 2-437 form when an ageing low-mass star — such as the Sun — reaches the final stages of life. The star swells to become a red giant, before casting off its gaseous outer layers into space. Hen 2-437 is a bipolar nebula — the material ejected by the dying star has streamed out into space to create the two icy blue lobes pictured here.
