Hubble Reveals a New Type of Planet
|GJ1214b, shown in this artist’s conception, is a super-Earth orbiting a red dwarf star 40 light-years from Earth. New observations from NASA’s Hubble Space Telescope show that it is a waterworld enshrouded by a thick, steamy atmosphere. GJ1214b therefore represents a new type of world, like nothing seen in our solar system or any other planetary system currently known. Credit: David A. Aguilar (CfA)|
Our solar system contains three types of planets: rocky, terrestrial worlds (Mercury, Venus, Earth, and Mars), gas giants (Jupiter and Saturn), and ice giants (Uranus and Neptune). Planets orbiting distant stars come in an even wider variety, including lava worlds and “hot Jupiters.”
Observations by NASA’s Hubble Space Telescope have added a new type of planet to the mix. By analyzing the previously discovered world GJ 1214b, astronomer Zachory Berta (Harvard-Smithsonian Center for Astrophysics) and colleagues proved that it is a water world enshrouded by a thick, steamy atmosphere.
“GJ 1214b is like no planet we know of,” said Berta. “A huge fraction of its mass is made up of water.”
GJ 1214b was discovered in 2009 by the ground-based MEarth (pronounced “mirth”) Project, which is led by CfA’s David Charbonneau. This super-Earth is about 2.7 times Earth’s diameter and weighs almost 7 times as much. It orbits a red-dwarf star every 38 hours at a distance of 1.3 million miles, giving it an estimated temperature of 450 degrees Fahrenheit.
In 2010, CfA scientist Jacob Bean and colleagues reported that they had measured the atmosphere of GJ 1214b, finding it likely that the atmosphere was composed mainly of water. However, their observations could also be explained by the presence of a world-wide haze in GJ 1214b’s atmosphere.
Berta and his co-authors used Hubble’s WFC3 instrument to study GJ 1214b when it crossed in front of its host star. During such a transit, the star’s light is filtered through the planet’s atmosphere, giving clues to the mix of gases.
“We’re using Hubble to measure the infrared color of sunset on this world,” explained Berta.
The super-Earth GJ 1214b, which has 6.5 times the mass of our Earth, orbits its star once every 38 hours at a distance of only 1.3 million miles. Astronomers estimate the planet¹s temperature to be about 400 degrees Fahrenheit. Although warm as an oven, it is still cooler than any other known transiting planet because it orbits a very dim star. Since GJ1214b crosses in front of its star, astronomers were able to measure its radius, which is about 2.7 times that of Earth. This makes GJ1214b one of the two smallest transiting worlds astronomers have discovered to date.
Credit: David A. Aguilar, CfA
Hazes are more transparent to infrared light than to visible light, so the Hubble observations help tell the difference between a steamy and a hazy atmosphere.
They found the spectrum of GJ 1214b to be featureless over a wide range of wavelengths, or colors. The atmospheric model most consistent with the Hubble data is a dense atmosphere of water vapor.
“The Hubble measurements really tip the balance in favor of a steamy atmosphere,” said Berta.
Since the planet’s mass and size are known, astronomers can calculate the density, which works out to about 2 grams per cubic centimeter. Water has a density of 1 g/cm3, while Earth’s average density is 5.5 g/cm3. This suggests that GJ 1214b has much more water than Earth, and much less rock.
As a result, the internal structure of GJ 1214b would be very different than our world.
“The high temperatures and high pressures would form exotic materials like ‘hot ice’ or ‘superfluid water’ — substances that are completely alien to our everyday experience,” said Berta.
Theorists expect that GJ 1214b formed farther out from its star, where water ice was plentiful, and migrated inward early in the system’s history. In the process, it would have passed through the star’s habitable zone. How long it lingered there is unknown.
GJ 1214b is located in the direction of the constellation Ophiuchus, and just 40 light-years from Earth. Therefore, it’s a prime candidate for study by the next-generation James Webb Space Telescope.
A paper reporting these results has been accepted for publication in The Astrophysical Journal and is available online: http://dx.doi.org/10.1088/0004-637X/747/1/35
This story has been translated into Portuguese.