KELT-24 (HD 93148, MASCARA-3) is a multiple star system in the constellation Ursa Major at a distance of approximately 316 light-years (about 96.9 parsecs) from Sun. The apparent magnitude of the primary star is +8.33. The star's age is estimated to be about 2.8 billion years. As an F-type main-sequence star, it is similar to the Sun, but slightly hotter, larger, and more luminous.
KELT-24 has a single known exoplanet, a hot Jupiter only 11 R☉ from the star.
This star was first catalogued in the Henry Draper Catalogue as HD 93148. The Henry Draper Catalogue gave stars visible to the naked eye in suitable conditions a designation, indicating that this star can be seen with the naked eye. But in 2019, the Multi-site All-Sky Camera and the Kilodegree Extremely Little Telescope announced the discovery of the exoplanet KELT-24b/MASCARA-3b around this star. Thus, it is most commonly known as KELT-24, although the star is sometimes catalogued as MASCARA-3. [6]
The common proper motion companion is referred to as HD 93148B or KELT-24B, [7] or KELT-24BC when it is being treated as a spectroscopic binary. [6]
KELT-24 is an 8th-magnitude F-type star with a faint companion separated by 2″ . The companion is over-luminous for a normal star of its colour and is suspected to be a binary consisting of two red dwarfs.
KELT-24 is a yellow-white star with a spectral class of F5. Its mass is about 1.3 M☉, its radius is about 1.5 R☉, and its luminosity is about 3.5 L☉. Its effective temperature is about 6,437 K . An age of 2.8 billion years has been calculated, but the 68% confidence interval ranges from 2.0 to 6.9 billion years. [6] Age estimates in the original discovery papers were 0.78 and 2.8 billion years respectively. [8] [9]
KELT-24B, or KELT-24BC when both components are being referred to, is suspected of being an eclipsing binary although only a single "transit-like event" has been observed. The best model fit is two near-identical red dwarfs each with a mass about half the Sun's and a luminosity less than 4% of the Sun's. [6]
In 2019, the discovery of the Hot Jupiter type planet KELT-24b/MASCARA-3b was announced by the Multi-site All-Sky CAmeRA and the Kilodegree Extremely Little Telescope. TESS data confirmed that no additional companions are orbiting this star. [10] [11]
Companion (in order from star) | Mass | Semimajor axis (AU) | Orbital period (days) | Eccentricity | Inclination | Radius |
---|---|---|---|---|---|---|
b | 4.6 MJ | 0.0501 | 5.5515 | 0.032 | 89.7° | 1.1 RJ |