From AAS NOVA: “Searching for Exoplanets Around X-Ray Binaries”



20 July 2018
Susanna Kohler

Artist’s impression of the first exoplanets discovered, which are in orbit around a magnetized neutron star, PSR B1257+12. A new study explores how we might find planets orbiting other compact objects — but compact objects that are accreting material from binary companions. [NASA/JPL-Caltech/R. Hurt (SSC)]

Finding planets around ordinary stars is great, but what if we could also hunt for planets around the black holes, neutron stars, and white dwarfs that live in binaries with companion stars? A new study shows it’s possible!

A New Place for Planets?

X-ray binaries are gravitationally interacting binary star systems in which a compact object — a white dwarf, neutron star, or black hole — accretes material from its companion star. In these systems, we can often detect the stars in optical or radio light, but the system additionally shines in X-rays as a result of radiation from the very hot, accreting gas.

Planets orbiting within binaries may be common — we’ve spotted around 70 examples so far of planets orbiting one member of a binary, and another dozen or so in which a planet orbits both members on a circumbinary path. It stands to reason, then, that some planets should survive the evolution of one of the binary stars into a compact remnant, eventually becoming a planet orbiting an X-ray binary.

Several example transit X-ray light curves for circumbinary planets, including an Earth-mass planet (solid lines) and a Jupiter-mass planet (dashed lines), for different values of μ, which relates the mass of the compact remnant to the companion star. Here the companion mass remains fixed and the different panels show different values for the remnant mass. [Imara & Dr Stefano 2018]

Looking at X-Rays

So how would we detect such a planet? Optical and radio searches for planets can be challenging, since a planet transit often means a very small dip in a light curve that might not be detectable. Two scientists from the Harvard-Smithsonian Center for Astrophysics, Nia Imara and Rosanne Di Stefano, propose an alternative: why not specifically look in the X-rays?

Because the area emitting X-rays is very compact — all smaller than the size of a white dwarf’s surface, i.e., the size of the Earth — the expected dip in the X-ray light curve due to a planet transit is quite large. This increases our chances of being able to detect it.

Exploring Challenges

A few challenges exist with this approach. To increase detection odds, the planet would ideally need to be orbiting within a similar plane to that of the binary, and preferably close to the inner cutoff for stable orbits around the binary. This is not an unreasonable assumption, however, given expected orbital dynamics as star systems evolve.

Transit probability versus binary mass ratio, μ, for planet circumbinary orbits around coplanar x-ray binaries with white dwarfs (solid lines), neutron stars (dashed lines), or black holes (dotted lines) as the primaries. The black and magenta lines represent the probability calculations for an Earth-like and Jupiter-like planet, respectively. [Imara & Di Stefano 2018]

Another potential difficulty is that X-ray photons are scarce! We’d have to observe systems for an extended time in order to gather enough light in X-rays to definitively detect light-curve dips. Imara and Di Stefano show, however, that we’ve observed a number of X-ray binaries over several hundred thousand seconds — long enough time periods that the dips would be detectable.

A Positive Outlook

With those challenges in mind, Imara and Di Stefano demonstrate through a series of calculations that circumbinary planets are reasonably likely to transit — transit probabilities range from roughly 0.1%–40%, depending on the mass ratio of the binary and the size of the X-ray-emitting region — and that our detection capabilities are such that we could actually spot these transits with present-day technology.

Future X-ray missions, like the proposed Lynx X-ray space telescope — which may have 50 times the sensitivity of the Chandra X-ray telescope! — will dramatically extend the opportunities for transit detection. Indeed, it seems like the hunt for these exotic exoplanetary systems have very good prospects.


Nia Imara and Rosanne Di Stefano 2018 ApJ 859 40.

See the full article here .


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