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XO-2

Binary star system in the constellation Lynx From Wikipedia, the free encyclopedia

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XO-2 is a binary star system about 490 light-years (150 parsecs) away in the constellation Lynx. It consists of two components, XO-2N and XO-2S, both of which host planetary systems.[10]

Quick facts Observation data Epoch J2000 Equinox J2000, Apparent magnitude (V) ...
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Star system

This system is unusual in that the stars are not typically referred to as components A & B, but are designated based on their positions in the sky: XO-2N is the northern star and XO-2S is the southern star.

Both of the stars are slightly cooler than the Sun and are nearly identical to each other. The system has a magnitude of 11 and cannot be seen with the naked eye but is visible through a small telescope. These stars are also notable for their large proper motions.[8][9]

XO-2N and XO-2S have a separation of approximately 4,600 AU.[3]

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Planetary systems

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There is one confirmed exoplanet orbiting XO-2N. XO-2Nb, which is classified as a hot Jupiter, was discovered by the XO Telescope using the transit method around XO-2N in 2007. It was initially the only known planet in the system and was referred to as XO-2b.[3] A long-period variation in the radial velocity of XO-2N was detected in 2015, which could be explained by either a second planet or a stellar activity cycle. The stellar activity explanation is considered more likely,[6] and is further supported by a 2024 study.[11]

Two planets were reported to orbit around XO-2S in 2014 using the radial velocity method. One of them is Jupiter-mass and another has a mass comparable to Saturn.[10] A 2024 study found evidence for a third, super-Jupiter mass planet around XO-2S.[11]

More information Companion (in order from star), Mass ...
More information Companion (in order from star), Mass ...
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See also

Other systems with multiple planet-hosting stars:

Notes

  1. Mass and eccentricity: Damasso et al. 2015[6]
    Other properties: Wang et al. (2025)[7]

References

Further reading

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