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Out of more than 3,000 clasts contained in the Chang’e-5 lunar sample, 7 do not come from the region of the Chang’e-5 landing sites. These exotic clasts highlight the lithological diversity of the lunar crust, and their scarcity hints at the need for alternative models for impact ejecta onto young lunar terrains.
Oxygen isotopic measurements from the Ryugu returned sample suggest that primitive hydrated carbonaceous chondrites are an important source of early water and other volatiles to Earth, despite being underrepresented in our meteorite collection due to their preferential destruction during atmospheric entry.
Infrared observations of Jupiter obtained in a 40-yr timespan between 1978 and 2019 show long-term variations of Jupiter’s tropospheric temperature with different periodicities, particularly at tropical latitudes, which often bear some connection with stratospheric temperature fluctuations.
A close-up look at the action of space weathering on carbonaceous asteroids, provided by Ryugu’s returned samples, highlights its role on the dehydration of the first micrometre-thick layer of the surface, possibly hiding a water-rich interior. The depth of the 2.7 µm hydration band may be an indication of the level of space weathering withstood by a C-type asteroid.
Wind power can be an oft-neglected source of energy for future human exploration missions on Mars, especially coupled with solar power. Modelling shows that solar and wind energy can fully power such missions for more than half of the Martian year for ten regions of interest identified by NASA. Another 13 promising sites are identified.
The ‘plane of satellite galaxies’ surrounding our Milky Way seemed to defy dark matter theory for 40 years. Observations now suggest that the alignment is transient, while new simulations form similar structures far more often than previously thought.
A comprehensive study of the Kepler-138 system reveals the twin nature of Kepler-138 c and d and the presence of a fourth planet. Remarkably, the warm-temperate planet Kepler-138 d is probably composed of 50% volatiles by volume, indicative of a water world, rather than a rocky world, despite its small ~1.5 R⊕ size.
A comparison of copper and zinc isotopic measurements between the Ryugu samples and various carbonaceous chondrites excludes any genetic link between the two except for the CI (Ivuna-type) chondrites. Ryugu-like material might have accounted for ~5% of Earth’s mass.
Observations of a meteoroid coming from the Oort cloud show that it is made of rocky and not icy material, constraining the ratio of rocky to icy objects impacting Earth from the Oort cloud to \({6}_{-5}^{+13}\)%.
A multi-observational study including laboratory analysis of the Chang’e-5 mission samples, in situ measurements and orbital datasets determined the high level of maturity and iron content of the Chang’e-5 landing site regolith. Heavily processed by space weathering, it mostly comes from the nearby Xu Guangqi crater, formed 240–300 Myr ago.
An ultraviolet- and carbon-rich environment is needed to explain the bright emission coming from complex organic molecules observed near the midplane of protoplanetary disks. This implies that the gaseous reservoir from which actively forming planets accrete is carbon and organic rich.
Measurements of the Rossiter–McLaughlin effect for the ultra-short-period super-Earth 55 Cancri e reveal a signal with a semi-amplitude of 0.41+0.09-0.10 m s−1, in close alignment with its star and potentially misaligned with the other planets in the system. Such a configuration favours a non-violent migration pathway for 55 Cnc e.
Simultaneous polarimetry measurements in the optical and radio bands for the afterglow emission of GRB 191221B provide insights into particle acceleration and total energy budget of gamma-ray bursts.
JWST observations of the planetary nebula NGC 3132 reveal a rich molecular environment containing evidence of multiple stellar interactions on a variety of scales.
Early emission from gamma-ray burst GRB 211211A comes entirely from charged particles accelerating in strong magnetic fields. The fast-evolving spectrum may be the key to understanding unusually long-lived GRBs from neutron star mergers.
Quantum sensors, such as atomic clocks, placed deep into the inner Solar system, may be sufficiently sensitive to directly detect ultralight dark matter bound by the mass of the Sun.
An ~4,000-km-diameter and 200–500-km-thick active mantle plume is present below Elysium Planitia on Mars, indicating that the Martian interior is geodynamically active and drives the volcanic and seismic activity of the region. Studies from the InSight lander need to consider the presence of the plume.
By modelling the radio, optical, UV and X-ray data of the unusually bright cosmological explosion AT 2022cmc, Pasham et al. argue for the presence of a highly collimated jet moving at ≳99.99% the speed of light.
An analysis of several models provides astrophysical constraints on the Universe at redshift ~20, corresponding to ~200 million years after the Big Bang, using upper limits on the sky-averaged 21-cm signal measured by the SARAS 3 radiometer.
Individual productivity among astronomers was boosted during the COVID-19 pandemic, but the improvement was not shared equally between men and women: a smaller fraction of papers were written by female astronomers and fewer women were among incoming new researchers in many countries.