In a first, scientists have identified the detailed chemical "fingerprint" of a planet between the sizes of Earth and Neptune to uncover clues about its nature and origin, using NASA's Sptitzer and Hubble space telescopes.
No planets like this can be found in our own solar system, but they are common around other stars, NASA said in a statement.
The planet, Gliese 3470 b (GJ 3470 b), may be a cross between Earth and Neptune, with a large rocky core buried under a deep, crushing hydrogen-and-helium atmosphere.
Weighing in at 12.6 Earth masses, the planet is more massive than Earth but less massive than Neptune, which is over 17 Earth masses.
Many similar worlds have been discovered by NASA's Kepler space observatory, whose mission ended in 2018. As many as 80 per cent of the planets in our galaxy may fall into this mass range.
However, astronomers have never been able to understand the chemical nature of such a planet until now, researchers said.
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By inventorying the contents of GJ 3470 b's atmosphere, astronomers are able to uncover clues about the planet's nature and origin.
"This is a big discovery from the planet-formation perspective. The planet orbits very close to the star and is far less massive than Jupiter -- 318 times Earth's mass -- but has managed to accrete the primordial hydrogen/helium atmosphere that is largely 'unpolluted' by heavier elements," said Bjorn Benneke of the University of Montreal in Canada.
"We don't have anything like this in the solar system, and that's what makes it striking," Benneke said.
Astronomers enlisted the combined multi-wavelength capabilities of Hubble and Spitzer space telescopes to do a first-of-a-kind study of GJ 3470 b's atmosphere.
This was accomplished by measuring the absorption of starlight as the planet passed in front of its star (transit) and the loss of reflected light from the planet as it passed behind the star (eclipse).
The space telescopes observed 12 transits and 20 eclipses. The science of analysing chemical fingerprints based on light is called "spectroscopy."
He hypothesizes that essentially it started out as a dry rock and rapidly accreted hydrogen from a primordial disk of gas when its star was very young. The disk is called a "protoplanetary disk."