Newfound Earth-size exoplanet has a scorching-hot lava side
NASA's Transiting Exoplanet Survey Satellite (TESS) has discovered an extraordinary planet that's roughly the size of Earth but is only one-tenth of our planet's age, with half of its surface likely dominated by scorching-hot lava.
The exoplanet orbits a sun-like star called HD 63433, which is located 73 light-years from Earth, at a proximity of around 12% the distance between Mercury and the sun. This is so close that the planet, designated HD 63433 d, completes an orbit in just 4.2 Earth days.
Because of this proximity to its star, which has 99% the mass of our sun, the planet is tidally locked, just like the moon is to Earth. This means that one side of the planet, its dayside, constantly faces the star and is permanently blasted with stellar radiation while the cooler nightside perpetually faces out into space. This pushes surface temperatures on the planet's dayside up around 2,300 degrees Fahrenheit (1,260 degrees Celsius), NASA officials said.
The violent temperatures of HD 63433 d mean that the planet's dayside is likely a hemisphere of blisteringly hot lava resembling that of exoplanets like CoRoT-7 b and Kepler-10 b.
However, this exoplanet is also remarkable for a slightly less extreme reason than its lava-dominated dayside.
HD 63433 d is also the smallest confirmed exoplanet that's less than 500 million years old. In addition to this, at 1.1 times the diameter of our planet, HD 63433 d is the closest roughly Earth-size planet to be discovered that is less than 400 million years old.
For comparison: Earth and the rest of our solar system are around 4.5 billion years old, meaning HD 63433 d appears to be just around 10% of the age of our planet.
The Earth-orbiting TESS discovered HD 63433 d as it crossed, or "transited," the face of its star, causing a slight dip in light from its stellar parent.
TESS, which launched in April 2018, has used this transit method of exoplanet detection to spot over 4,000 alien worlds, of which several hundred have been confirmed.
This isn't the first planet to be discovered orbiting HD 63433; the existence of sibling worlds prompted further investigation of the system. In 2020, the transit method uncovered HD 63433 b and HD 63433 c. The former is a roughly Neptune-size planet around 2.1 times wider than Earth and roughly five times more massive. HD 63433 b orbits its star at 0.07 times the distance between Earth and the sun, with a year that lasts 7.1 Earth days.
HD 63433 c is slightly larger, around 0.23 times the size of Jupiter, with a mass around seven times that of Earth. This world takes a relatively leisurely orbit of 20.5 Earth days around its star, dwelling at a distance 0.14 times that between Earth and the sun.
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The unique features of HD 63433 make it a primary target for subsequent investigations that will aim to further study both the day and night hemispheres of this world.
The discovery of HD 63433 d was discussed on Wednesday (Jan. 10) at the 2024 American Astronomical Society Meeting in New Orleans, Louisiana, and is detailed in a paper published that same day in The Astronomical Journal.
