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Kepler-93b

Kepler-93b (KOI-69b) is a hot, dense transiting Super-Earth exoplanet located approximately 313 light-years (96parsecs)^[4] away in the constellationofLyra,^[5][6] orbiting the G-type star^[5] Kepler-93. Its discovery was announced in February 2014 by American astronomer Geoffrey Marcy and his team.^[1] In July 2014, its radius was determined with a mere 1.3% margin of error, the most precise measurement ever made for an exoplanet's radius at the time.^[7]

Physical properties[edit]

The planet has a radius of around 1.478 R_🜨 (9,416 km), with an uncertainty of just 0.019 R_🜨 (121 km),^[8] making it the most precisely measured exoplanet ever in terms of radius as of July 2014.^[7] The planet is substantially denser than Earthat6.88±1.18 g/cm^3[9] thanks to its high mass of roughly 4 M_E, consistent with a rocky composition of iron and magnesium silicate.^[9] In 2023, the planet's mass was revised upward to 4.66±0.53 M_E, placing its density at 7.93^+0.96
_−0.94 g/cm³,^[3] roughly the same as the metal iron (7.874 g/cm³).^[10]

Based on these findings, the interior of the planet is likely similar to that of Earth and Venus, with an iron core making up around 26% of its total mass (albeit with a large uncertainty of ±20%),^[11] compared to the 32.5 ± 0.1% of Earth and 31 ± 1% of Venus.^[11]

The planet orbits its host star every 4.73 days^[8] at a distance of 0.05343 AU (7,993,000 km),^[3] less than one-seventh the radius of Mercury's orbit. Its equilibrium temperature is approximately 1,133 K (860 °C; 1,580 °F),^[3] which is as hot as lava and well above the melting pointofaluminium.^[a]

Host star[edit]

The planet orbits a Sun-like (spectral type G5V)^[5] star named Kepler-93. The star has a mass of 0.911 M_☉ and a radius of 0.919 R_☉. It has a temperature of 5,669 K (5,396 °C; 9,745 °F) and is 6.6 billion years old.^[8] In comparison, the Sun is 4.6 billion years old,^[14] has a temperature of 5,772 K (5,499 °C; 9,930 °F) and a spectral type of G2V.^[15] The apparent magnitude of the star is 9.931,^[9] making it too dim to be visible from Earth by the naked eye.^[16]

The star is host to an additional non-transiting confirmed companion, Kepler-93c, which was discovered using the radial-velocity method and announced in 2014, concurrently with Kepler-93b.^[1] The object is most likely a brown dwarf orbiting much farther out than Kepler-93b, though its precise nature remains uncertain. The discovery paper reported a lower limit on the mass of 3 M_J and a minimal orbital period of 1,460 days (4.0 years),^[1] while a subsequent study in 2015 weighed the planet at >8.5 M_J and presented an orbital period of >10 years, placing its orbit beyond 4.5 AU from the star,^[9] and a 2023 study increased these lower limits further, to a mass >21M_J, an orbital period >48.6 years, and a semi-major axis >13 AU.^[3]

See also[edit]

• List of exoplanets discovered by the Kepler space telescope
• List of transiting exoplanets
• Other dense super-Earths orbiting close to their parent stars:
  • CoRoT-7b, has a similar radius to Kepler-93b, but is more massive and much hotter.
  • HD 219134 b, has a similar radius, mass and temperature.
  • Kepler-10b, has a similar radius, but is slightly less massive and much hotter.
  • Kepler-36b, has a similar radius, mass and temperature.

Footnotes[edit]

References[edit]