A Short Period

In Black Holes by Brian Koberlein0 Comments

In the center of our galaxy, only 27,000 light years away, lies a supermassive black hole.  Some of the strongest evidence of this black hole is the observation of stars closely orbiting it.  I’ve plotted the orbits of a few of these in an earlier post.  At the time, the star with the shortest orbital period was S0-2, with a period of about 15.5 years.  Recently in Science a new star, S0-102, was announced with an period of 11.5 years.  You can see a plot of this new star in the figure below.

F2.largeTwo things make this announcement interesting.  The first is that it is part of a process of discovering more stars orbiting the supermassive black hole. Observing these stars is hard, because they are obscured from our direct view by gas and dust surrounding the center of our galaxy.  We have to infer their positions by infrared and radio observations.  Until recently, we’ve only been able to get good measurements on the brightest of these stars.  However by observing the motion of the bright stars, we’ve been able to determine the mass of the supermassive black hole fairly well.  This means we can use its mass to predict the motion of orbiting stars.  These predictions allow us to refine observations of dimmer stars such as S0-102.  By observing brighter stars, we can find dimmer stars with confidence.

The second interesting aspect is that it provides an observational test of general relativity.  Stars such as S0-2 and S0-102 orbit the black hole so closely that their orbits should precess due to the curvature of space and time.  Given the shortness of their periods, we should be able to observe this precession directly.
Of course the most interesting aspect is that we can actually watch stars falling around a black hole.  How cool is that?

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