WISPIT 2 (also called TYC 5709-354-1) is a binary star in the constellation Aquila. It is part of the Scorpius-Centaurus OB association, likely belonging to the subgroup Theia 53. The system has a directly imaged circumstellar disk with multiple rings and two directly imaged protoplanets inside the rings' gaps. One of the protoplanets, WISPIT 2b, was also detected in H-alpha, showing that it is actively accreting gas from a surrounding circumplanetary disk. The star is named after the astronomical survey Wide Separation Planets In Time (WISPIT) in the course of which the protoplanetary system was discovered. The binary nature of WISPIT 2 was discovered in 2026. It is a single-lined spectroscopic binary with an orbital period of 4.8 days a semi-major axis of 0.072 au. The orbit is thought to be circular, with an eccentricity close to zero, and the inclination is assumed to be the same of the outer disk, based on observational evidence. The primary has an estimated mass of 0.97 M☉, while the estimated mass of the secondary is 0.33 M☉.
Circumstellar disk The disk was classified as transitional, meaning it has an inner cavity. The disk has 4 rings and one prominent gap at 68 astronomical units (AU). The outermost ring is located at 316 AU and the disk was detected out to a distance of 2.8 arcseconds (380 AU) from the star. The inclination of the disk is around 44° to 46°.
Planetary system Observations with VLT/SPHERE, Magellan MagAO-X and LBT/LMIRcam revealed one planet located inside gap 3. The protoplanet was confirmed to move with the star and shows orbital motion in images from October 2023 to April 2025. The planet has a mass of around 5 MJ and is responsible for clearing a gap inside the disk. The protoplanet is also detected in H-alpha, showing that it is accreting material from a circumplanetary disk. This makes WISPIT 2b similar to the PDS 70 planets, 2MJ1612b and possibly LkCa 15b.
One additional inner candidate planet, CC1, was detected together with WISPIT 2b, but needed further observations to determine whether it is a planet or a dust clump. Spectroscopic observations published in 2026 confirmed that CC1 is indeed a planet, now named WISPIT 2c.
See also List of directly imaged exoplanets WISPIT 1
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