"You could lose, or at least completely fry, rocky planets forming close to such a star." ...
Researchers using NASA's Hubble Space Telescope have discovered that the accretion disk around the young star FU Orionis is ...
In 1936 astronomers watched as FU Orionis, a dim star in the Orion constellation, brightened dramatically. The star’s ...
Ultraviolet light reveals new information about the FU Orionis' mechanisms. In 1936, the young star FU Orionis (FU Ori) ...
The findings reveal that the inner disk touching the young star is extraordinarily hot, challenging conventional ...
NASA's Hubble reveals FU Orionis’s disk burns at 16,000 Kelvin, three times the Sun's heat, altering planet formation ...
First observed in 1936, FU Orionis became a hundred times brighter in months and has remained a unique object of study.
This is an artist's concept of the early stages of the young star FU Orionis (FU Ori) outburst, surrounded by a disk of ...
In 1936, astronomers saw a puzzling event in the constellation Orion: the young star FU Orionis (FU Ori) became a hundred ...
In 1936, astronomers saw a puzzling event in the constellation Orion: the young star FU Orionis (FU Ori) became a hundred times brighter in a matter of months. At its peak, FU Ori was ...