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Planetary science has long enjoyed an important role in Nature history.
Nature has published many important advances since the beginning of space exploration, from a seminal series of papers on Giotto observations of comet Halley, to the detection of the first Kuiper belt object, the presentation of the Grand Tack theory and the first results of the Huygens probe that landed on Titan in 2005, just to name a few.
This collection aims to highlight just a few of the discoveries in planetology published by Nature Research in the past three years. Five different journals contribute to this collection (Nature, Nature Geoscience, Nature Physics, Nature Chemistry and Nature Communications), demonstrating the widespread interest and the great diversity of themes presented in our pages.
Nature Astronomy, a new member of the Nature family set to launch in January 2017, welcomes planetary science as an important part of its scope and will be the latest addition to this great tradition.
This collection is formed by six main sections, each dedicated to a different theme or target: Comparative planetology, Mars' surface flows, Dwarf planets, Comets-asteroids, Moons, and Gas giant planets. The sections contain a small set of manuscripts illustrating the Nature output in the various fields. Different types of publications are represented, from standard Articles and Letters, to the various other formats, including News & Views, Commentaries and Reviews, which the Nature journals propose to the scientific community as companion pieces for a more in-depth analysis and discussion on the published original research.
Articles on the Research and Comment pages are freely available to access for a limited time.
The Pluto image in the header is from NASA/JHUAPL/SwRI.
This year, NASA's Dawn and New Horizons rendezvoused with Ceres and Pluto, respectively. These worlds, despite their modest sizes, have much to teach us about the accretion of the Solar System and its dynamical evolution.
Planets are no longer the only Solar System bodies sporting ring systems. Two dense rings have been detected encircling a Centaur object — a relatively small, icy interloper from the distant reaches of the Solar System. See Letter p.72
Data obtained by the Cassini spacecraft show that the plume of ice particles at the south pole of Saturn's moon Enceladus is four times brighter when the moon is farthest away from the planet than when it is closest. See Letter p.182
In the second of two essays looking at organic chemistry that can be found in the Solar System, Bruce C. Gibb focuses on the gas and ice giants as well as their satellites — concluding the tour on Saturn's fascinating moon Titan.
Gas-giant planets are widely thought to form from solid ‘cores’ of roughly ten Earth masses; simulations now show that such cores can be produced from ‘pebbles’ (centimetre-to-metre-sized objects) provided that the pebbles form sufficiently slowly, leading to the formation of one to four gas giants in agreement with the observed structure of the Solar System.
Observations of a stellar occultation by (10199) Chariklo, a minor body that orbits the Sun between Jupiter and Neptune, reveal that it has a ring system, a property previously observed only for the four giant planets of the Solar System.
The plume at the south pole of Enceladus is several times brighter when that moon is near the apocentre of its eccentric orbit around Saturn than when it is near its orbital pericentre, showing that more material appears to be escaping from beneath Enceladus’ surface at times when models predict its fissures should be under tension.
Transient streaks that appear seasonally on Martian slopes are consistent with brine flows, but evidence of water or salts has been lacking. Analysis of spectral data reveals hydrated salts associated with the streaks, confirming a briny origin.