Planets

Blog about planets.

A diagram of a secondary eclipse and a graph of the resulting change in brightness over time in the 55 Cancri system based on detections by the James Webb Space Telescope's MIRI instrument

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An article published in the journal “Nature” reports the results of a study of the exoplanet 55 Cancri e, formally called Janssen, which confirms the presence of an atmosphere that is considered secondary, which means that it derives from emissions coming from the planet itself. A team of researchers led by NASA’s Jet Propulsion Laboratory (JPL) used observations conducted with the James Webb Space Telescope to detect traces of an atmosphere that may be rich in carbon monoxide or carbon dioxide.

Artist's concept of the impact of a dwarf planet on Pluto (Image courtesy University of Bern, Illustration: Thibaut Roger)

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An article published in the journal “Nature Astronomy” offers an explanation for the formation of the large and deep basin known as Sputnik Planitia on Pluto with its characteristic heart shape. A team of scientists coordinated by the Swiss University of Bern created computer simulations that indicate that the depression that is some kilometers deep could have been generated by an impact with an object with a diameter of around 700 kilometers that occurred at an oblique angle and was relatively slow. The results of these simulations also suggest that Pluto likely doesn’t have a subsurface ocean of liquid water, unlike other studies.

Dantu crater on the dwarf planet Ceres (Image courtesy Maria Cristina De Sanctis et al., Communications Earth & Environment, 2024)

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An article published in the journal “Communications Earth & Environment” reports the discovery of ammonium-rich areas in the famous bright spots on the dwarf planet Ceres. A team of researchers composed of Maria Cristina De Sanctis, Filippo Giacomo Carrozzo, Mauro Ciarniello, Simone De Angelis, Marco Ferrari, Alessandro Frigeri, and Andrea Raponi from the Italian National Institute of Astrophysics’ Institute of Space Astrophysics and Planetology in Rome and Eleonora Ammanito of the Italian Space Agency examined data collected by NASA’s Dawn space probe focusing on Dantu crater to identify these compounds, which include a new ammonium salt.

Some of the systems observed with the VLT and represented here not in scale to appear similar in size

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Three articles published in the journal “Astronomy & Astrophysics” report different aspects of a large study of 86 protoplanetary disks located in three different regions of the Milky Way. Teams of researchers with several shared members used the SPHERE instrument mounted on ESO’s Very Large Telescope (VLT) in Chile as part of the GTO and DESTINYS observation programs. The findings offer a treasure trove of information about planetary formation in the cosmic neighborhood that could lead to advances in current models and aid follow-up studies.

Artist's concept of the exoplanet TOI-715b with its star in the background (Image NASA / JPL-Caltech)

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An article published in the journal “Monthly Notices of the Royal Astronomical Society” reports the identification of the exoplanet TOI-715 b in an orbit around its star in a position that meets the most conservative definition of a habitable zone. A team of researchers used observations conducted with NASA’s TESS space telescope confirmed by other instruments to identify what appears to be a super-Earth with a radius about 1.5 times the Earth’s. A second exoplanet candidate was discovered that would have a size very similar to the Earth’s a little further away from its star but follow-up observations are needed to verify that it’s not a false positive.