Measuring the mass of a single star
In the image at top, left, astronomers discovered a subtle brightening of a star [located within the box] due to the effect of gravitational microlensing. This phenomenon occurs when a foreground star, in this case a dim red star, passes in front of a much more distant star and amplifies its light. Astronomers were engaged in a large-scale search for microlensing events in the halo of our Milky Way galaxy. They were looking in the direction of the Large Magellanic Cloud, a satellite galaxy of our Milky Way. The image was taken in February 1993 with the 50-inch telescope at the Mount Stromlo Observatory in Australia. The box represents the field of view of NASA/ESA Hubble Space Telescope.
Credit:About the Image
About the Object
Name: | MACHO-LMC-5 1994 |
Type: | Milky Way : Cosmology : Phenomenon : Lensing Local Universe : Star Milky Way : Star |
Category: | Stars |
Colours & filters
Band | Wavelength | Telescope |
---|---|---|
Optical V | 606 nm |
Hubble Space Telescope
ACS |
Infrared I | 814 nm |
Hubble Space Telescope
ACS |
Notes: This image was captured with the 50-inch telescope at the Mount Stromlo Observatory.