Baby Jupiter Discovery a Step Toward Rewriting Planet Formation Models

Exoplanet 51 Eridani b
An artist's conception of exoplanet 51 Eridani b, which resembles a very young Jupiter could help scientists write a new theory of planet formation. (Image credit: Danielle Futselaar and Franck Marchis, SETI Institute)

Over the last two decades, the discovery of thousands of exoplanets outside our solar system has shaken up old theories about how planets form;the recent discovery of an "infant Jupiter," rich in methane, may be one step toward writing a new one.

A very young gas giant planet called 51 Eridani b, located 96 light-years from Earth, has a methane-rich atmosphere, just like Jupiter. This is a first, according to a statement from Stanford University: the handful of gas giant atmospheres that scientists have been able to study contain only trace amounts of methane, despite what scientists anticipate for those types of planets. 

How does this methane discrepancy arise? It may be due to the effects of a planet's environment over time, but it may also be a difference in how these giants formed. The Gemini Planet Imager (GPI), which directly imaged 51 Eridani b and measured the methane in its atmosphere, is looking at extremely young gas giants to help figure out what happens in the planetary womb to create the wide range of planets that scientists now observe. [Jupiter-Like Exoplanet With Methane Atmosphere Found | Video]

Exoplanet 51 Eridani b, a world only 20 million years old and still hot from its creation, has been photographed in a solar system 96 light-years from Earth. Learn all about 51 Eridani b in our full infographic. (Image credit: By Karl Tate, Infographics Artist)

Planet formation, fast and slow

Planets don't radiate light the way stars do, but they're not entirely dark, either. Planet 51 Eridani b, for example, burns at about 800 degrees Fahrenheit (426.6 degrees Celsius), which is hot enough to melt lead and give off a substantial glow.

The heat comes from energy that was captured during the planet's formation process, which took place about 20 million years ago. Jupiter is closer to 4.5 billion years old, so by contrast, 51 Eridani b is a planetary infant.

"It's young enough to remember how it formed," said Bruce Macintosh, principal investigator of GPI (which Macintosh pronounces "gee-pie," but which some of his colleagues pronounce "gee-pee-eye"). "The details of its formation process affect how bright it is."

The GPI instrument was designed to search for young gas giants. It directly detects the light radiated by these hot, young things, whereas the Kepler Space Telescope (which has identified more than 4,000 planet candidates), finds planets by watching for the dip in the brightness of a star as the planet passes in front of it.

"To detect planets, Kepler sees their shadow," Macintosh said in the statement from Stanford University. "The Gemini Planet Imager instead sees their glow, which we refer to as direct imaging."

According to Macintosh, the brightness or temperature of a young planet could reveal how that planet formed.

There are two key ideas as to how massive gas planets form: fast or slow.

The fast-formation method suggests that the material rapidly coalesces into a hot, mixed-up ball of gas and solid material, Macintosh said. By contrast, Jupiter is thought to have formed via the slow formation process, which starts with the gradual buildup of a rocky core, followed by the rapid accretion of gassy outer layers. If the latter process is very slow, it may stop short of gaining the gassy layers, and form a rocky planet like Earth.

"Planets are not as bright if they form slow. If the planet forms fast, then a lot of energy gets trapped inside it," Macintosh told "If you measure the brightness of a planet, you can maybe tell which formation pathway it follow."

According to the statement from Stanford, other Jupiter-like exoplanets discovered thus far have been "much hotter" (that is, brighter) than slow-formation models predict they should be. The GPI team hasn't yet made a definitive measurement of 51 Eridani b's brightness (to do this they must also measure its mass), but the detection of methane has raised the team's hopes about what this new, methane-rich planet will tell them about the formation of other, Jupiter-like planets in the universe.

Macintosh said it is possible that both the fast and slow formation processes take place in the universe. If that is true, he said, then scientists will want to understand how frequently each process tends to occur, because that would also influence how frequently small, rocky planets form.

"The planets in our solar system formed slowly, maybe most of the Kepler planets formed fast," Macintosh said. "What percentage of planets don't get caught up in that fast system?" [The 6 Most Earth-Like Alien Planets]

: Discovery image of the exoplanet 51 Eridani b was taken in the near-infrared light with the Gemini Planet Imager on Dec. 21, 2014. The bright central star has been mostly removed to enable the detection of the million-times fainter planet. (Image credit: J. Rameau (UdeM) and C. Marois (NRC Herzberg))

GPI and future telescopes

The GPI instrument is about the size of a subcompact car, and rests on top of the 8-meter Gemini South Telescope in Chile. It is built to specifically study young gas giants like 51 Eridani b.

Twenty years ago, planet scientists had what seemed like a solid model of planet formation, Macintosh said, before telescopes revealed a whole swath of exoplanet solar systems that evolved very differently from our own. The old model couldn't explain, for example, how massive gas giant planets could be located extremely close to their parent stars, and yet that kind of arrangement has been found with some frequency. With an updated theory of planet formation, Macintosh said, scientists have a better chance of using such a model to help them search for more planets, including rocky, Earth-like ones.

"Once that model traces the top of the iceberg, the visible part, then you can see what it predicts about the invisible parts of the system. The planets you can't see," he said.

A better model of planet formation would also, in theory, help scientists better understand systems that contain planets that sit on the border between gaseous and rocky: those that could be either "super-Earths" or "mini-Neptunes." A planet formation model would provide information about which types of planets are more likely to form, under what conditions, and what other indicators might be present that could help scientists determine a planet's makeup.

The GPI instrument will never be able to see rocky planets directly ­— they would be far too small and too dim. But many of the instruments that GPI uses to find young gas giants might be added to the Wide-Field Infrared Survey Telescope (WFIRST) space observatory, set to launch in the mid-2020s, which will study dark matter and search for exoplanets. As such, GPI is serving as a test bed for some of those technologies, and is paving the way for more direct hunts for Earth-like planets that may host life.

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Calla Cofield
Senior Writer

Calla Cofield joined's crew in October 2014. She enjoys writing about black holes, exploding stars, ripples in space-time, science in comic books, and all the mysteries of the cosmos. Prior to joining Calla worked as a freelance writer, with her work appearing in APS News, Symmetry magazine, Scientific American, Nature News, Physics World, and others. From 2010 to 2014 she was a producer for The Physics Central Podcast. Previously, Calla worked at the American Museum of Natural History in New York City (hands down the best office building ever) and SLAC National Accelerator Laboratory in California. Calla studied physics at the University of Massachusetts, Amherst and is originally from Sandy, Utah. In 2018, Calla left to join NASA's Jet Propulsion Laboratory media team where she oversees astronomy, physics, exoplanets and the Cold Atom Lab mission. She has been underground at three of the largest particle accelerators in the world and would really like to know what the heck dark matter is. Contact Calla via: E-Mail – Twitter