James Webb Space Telescope Discovery

JWST reveals details of the atmospheric composition of the Mini-Neptune GJ 1214 b

The James Webb Space Telescope reveals details of the atmospheric composition of the Mini-Neptune GJ 1214 b: after almost 15 years of futile efforts, an international team of researchers involving the Max Planck Institute for Astronomy has determined some of the atmosphere’s properties of the exoplanet GJ 1214 b. To this end, astronomers have now measured the infrared radiation of the planet classified as a sub-Neptune with the MIRI spectrograph of the James Webb Space Telescope and evaluated it with the help of model calculations. The results indicate an unusually highly reflective, dense haze in the upper atmosphere and show evidence of water vapour and methane. Artist’s impression of the exoplanet GJ 1214 b, based on the current results. GJ 1214 b is a warm mini-Neptune with a perpetual day on one side and eternal night on the other. An unusually reflective haze layer in the upper atmosphere makes it difficult to determine the composition of the sheets below. The planet probably has large amounts of water. NASA/JPL-Caltech/R. Hurt (IPAC) “Our results show that the haze layer of GJ 1214 b must have a composition different from known celestial bodies,” says Maria Steinrueck from the Max Planck Institute for Astronomy in Heidelberg, Germany. She is a an author of the paper, which appears in the journal Nature, and performed the model calculations essential for evaluating the observations. A dense, highly reflective veil The data can only be explained by the researchers’ assumption of a layer in the planet’s upper atmosphere that reflects the radiation from the central star, which GJ 1214 b orbits once in 38 hours, unusually well. Exactly what this layer consists of, however, remains a mystery, as none of the compositions suspected so far provides a satisfactory explanation. At least, the usual candidates have been ruled out. “Neither soot particles nor so-called tholins reflect the star’s radiation sufficiently strongly,” Steinrueck states. The term “tholin”, coined by the Planetary Scientist Carl Sagan, describes a variable mixture of hydrocarbons found on Saturn’s moon Titan and other bodies in the Solar System. Presumably, the atmosphere of the primordial Earth also consisted partly of tholins. Evidence of water The new observations with MIRI (Mid-Infrared Instrument) on board the James Webb Space Telescope for the first time also prove that the atmosphere beyond hydrogen and helium must have a high fraction of heavy elements. This follows from the model calculations that reproduce the measured variation in brightness of the starlight reprocessed by the planet. This image illustrates how a star illuminates and heats the day side of a tidally locked planet orbiting in bound rotation. Similar to how we see Venus in the solar system, such a planet shows different fractions of its day and night sides, the phases, during an orbit. In observing GJ 1214 b, astronomers tracked the planet’s signal as a function of the degree of illumination, obtaining data of the entire planet. ESA With their observations, the astronomers have captured a complete orbit of GJ 1214 b and thus measured its surface from all sides – a first for a Mini-Neptune. The light GJ 1214 b receives from its central star serves as a probe. Any interactions of the planet with the starlight will then show up in fluctuating proportions of the planet’s radiation. The measurement data also indicate the concrete composition of the atmosphere. As already suspected, this planet probably has water, which appears as gaseous vapour. “GJ 1214 b could therefore be a water world,” says Eliza Kempton, professor at the University of Maryland, USA and leading author of the research article. However, the features could also indicate methane gas. A mixture of both is also conceivable. Further observations are therefore needed to clarify the matter. A planet with eternal day and night In 2009, astronomers discovered GJ 1214 b, just under 50 light years away, using the transit method. In this method, the planet’s orbit is oriented in such a way that it regularly crosses its central star, and the occultation slightly reduces the star’s brightness. This measurement made it possible to calculate its size of 2.5 to 3 Earth diameters. Its mass is about seven Earth masses, classifying GJ 1214 b as a Mini-Neptune. This type of exoplanet is the most common one that astronomers find. However, there are no such planets in the Solar System. That is one reason why their nature is poorly known. GJ 1214 b orbits its central star, GJ 1214, at a distance of about one-seventieth of the distance between the Earth and the Sun. This means that the planet is in a so-called tidally locked rotation. In other words, it takes the same time to orbit the host star as the planet needs to rotate around its axis. Consequently, the host star always illuminates and heats the same side of the planet. Winds carry the air to the opposite hemisphere, where it cools in eternal night. Heat map of the exoplanet GJ 1214 b obtained by analysing the infrared radiation collected by the MIRI spectrograph on the JWST. Like a world map, it shows a projection of the entire surface. The planet always faces the star on the same side. Thus, the star is vertically above the point corresponding to zero longitude and latitude. The temperature is given in Kelvin (0 degrees Celsius = 273.15 Kelvin). It results from the assumption that the measured radiation originates from a completely black body without atmosphere. The actual temperature is modified from the additional atmospheric influence. The black sector -120 degrees longitude indicates a range of low temperature in which the data are too unreliable for a meaningful temperature to be assigned to them. Eliza M.-R. Kempton et al. / MPIA As with Earth’s global climate, the temperature on GJ 1214 b depends on various influences: the luminosity and temperature of the star, the distance of the planet from the star and the properties of the atmosphere. This results in a characteristic thermal radiation of the planet, which the researchers recorded with the MIRI observations. These consist of spectra that split the different parts of the infrared radiation according to their wavelength. As a result, the astronomers conclude that the haze reflects half of the radiation from the central star without contributing to the heating of the atmosphere. The calculations thus show that GJ 1214 b has an average global temperature of about 230 degrees Celsius (500 Kelvin), which varies by about 115 degrees between day and night. Credit: Max Planck Institute