Research alert! Rebecca Oppenheimer, a curator in the Museum’s Department of Astrophysics, co-discovered the first brown dwarf, Gliese 229B, in 1995. Since then, there’s been a long-standing mystery: Why does this brown dwarf shine so faintly despite having a significant mass—70 times that of Jupiter?
The answer, which is detailed in her latest study with Caltech—out today in the journal Nature—is that this brown dwarf is actually two objects, orbiting very closely around each other.
“These two worlds whipping around each other are actually smaller in radius than Jupiter. They’d look quite strange in our night sky if we had something like them in our own solar system,” Oppenheimer said. The discovery leads to new questions about how tight-knit brown dwarf duos like this one form and suggests that similar systems are likely out there. Read more.
Image: K. Miller, R. Hurt (Caltech/IPAC)