Planets

Artistic representation of the exoplanet WASP-193 b

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An article published in the journal “Nature Astronomy” reports the identification of the exoplanet WASP-193 b, a gas giant whose diameter is approximately 1.5 times Jupiter’s but with a mass that is only one-seventh of Jupiter’s. A team of researchers led by Khalid Barkaoui of the University of Liège, Belgium, used the WASP-South telescope of the Wide Angle Search for Planets (WASP) collaboration to locate WASP-193 b and then study its characteristics with other instruments. The combination of this exoplanet’s mass and density is really difficult to explain since no theory of planetary formation leads to a planet like this.

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.