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The Sun observed across eight different wavelengths by the Solar Orbiter space probe

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ESA has released the first information, including the first images, of the Sun’s South Pole, captured between March 16 and 17, 2025, by the Solar Orbiter space probe, a mission operated in collaboration with NASA. Three of the scientific instruments on board made it possible to observe that area in different electromagnetic bands: Polarimetric and Helioseismic Imager (PHI), Extreme Ultraviolet Imager (EUI), and Spectral Imaging of the Coronal Environment (SPICE). The Sun’s poles aren’t visible from Earth, and Solar Orbiter is observing them as never before. The first observations have already revealed some surprises.

ASKAP J1832-0911 (in the circle) (Image X-ray: NASA/CXC/ICRAR, Curtin Univ., Z. Wang et al.; Infrared: NASA/JPL/CalTech/IPAC; Radio: SARAO/MeerKAT; Image processing: NASA/CXC/SAO/N. Wolk)

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An article published in the journal “Nature” reports a study on ASKAP J1832-0911, or simply ASKAP J1832, an object whose nature is still uncertain. A team of researchers combined data collected by different instruments, including NASA’s Chandra X-ray Observatory and the ASKAP radio telescope, to detect the emissions coming from this object. This allowed them to reveal anomalies with respect to the categories considered to try to identify it.

The radio emissions led to cataloging it as a long-period radio transient, but ASKAP J1832 has variable emissions of the same duration in X-rays as well. An object with that type of emissions has never been found before, so it arouses a lot of curiosity. It could be a magnetar or a white dwarf with a companion star, but its behavior remains strange, so the investigations will continue.

The Magellanic Clouds as seen by the Gaia space probe (Image ESA)

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An article published in “The Astrophysical Journal Letters” reports the results of a study of the Small Magellanic Cloud that shows how this dwarf galaxy is undergoing distortions in its shape due to various gravitational influences. Satoya Nakano and Kengo Tachihara of Nagoya University, Japan, used data collected by ESA’s Gaia space probe together with information on Cepheid stars collected by the OGLE (Optical Gravitational Lensing Experiment) project. This allowed them to determine the distances of 4,236 Cepheids and the anomalies in their motions. The conclusion is that the Small Magellanic Cloud is undergoing a gravitational influence from the Large Magellanic Cloud and another as yet unknown source.

On the left the supernova SN 1987A remnant as seen by the James Webb Space Telescope, and in the other two panels the simulation of the density distribution of the remnant, which include the iron-rich materials, and the current morphology of that remnant

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An article to be published in the journal “Astronomy & Astrophysics” reports a study of the supernova SN 1987A that offers evidence that the explosion was decidedly asymmetric and dominated by two bipolar jets. A team of researchers led by astrophysicist Salvatore Orlando of the Italian National Institute of Astrophysics in Palermo has developed a model that takes into account the interaction between matter and magnetic field to study the evolution of SN 1987A. The results successfully reproduce the morphology of the iron-rich ejected materials, which was observed in particular by the James Webb Space Telescope. This shows that those structures are the result of an asymmetric explosion.

15 protoplanetary disks studied in the ODISEA project with their classification according to the proposed model

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An article published in “The Astrophysical Journal Letters” reports a model that traces the evolution of protoplanetary disks through five stages. A team of researchers from the ODISEA (Ophiuchus DIsc Survey Employing ALMA) project developed this model using both simulations and observations of protoplanetary disks within the Ophiuchus molecular cloud obtained using the ALMA radio telescope. The type of evolution observed confirms the division into stages proposed in 2020 in an article published in the journal “Monthly Notices of the Royal Astronomical Society” and offers some confirmation of the mechanisms by which giant planets influence the dynamics within those disks.