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Volume 8 Issue 1, January 2024

Habitability across geological timescales

Habitability is usually defined for a specific time during a planet’s evolution. But how is that habitability sustained over billions of years? Comparing habitable conditions across different Solar System bodies is key to our understanding of the underlying processes driving long-term habitability.

See Cockell et al.

Image: James Tuttle Keane, Jet Propulsion Laboratory, California Institute of Technology. Cover design: Bethany Vukomanovic.

Editorial

  • A series of pieces published in this issue highlights the breadth and depth of topics discussed in modern astrobiology, an exciting discipline that has come to the forefront of astronomy in recent years and promises to answer one of the most fundamental questions of humanity.

    Collection:

    Editorial

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Correspondence

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Comment & Opinion

  • Is the scientific status of astrobiology undermined by the lack of evidence for alien life, the problematic influence of science fiction, or the use of ‘astrobiology’ as a buzzword for attracting funding? Here we defend the emerging discipline.

    • Cyrille Jeancolas
    • Catherine Gillen
    • Peter Vickers

    Collection:

    Comment
  • The search for life elsewhere involves variables across multiple scales in time and space, often nested hierarchically. We suggest that the emergence of artificial intelligence learning systems offers critically important ways to make progress.

    • Caleb A. Scharf
    • Marisa H. Mayer
    • Penelope J. Boston

    Collection:

    Comment
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Research Highlights

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News & Views

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Research Briefings

  • Theories predict that core asphericity must be involved in core-collapse supernova explosions; however, the shape of these explosions has not been directly observed. The distribution of the explosive burning ash has now been revealed using nebular spectroscopy, indicating that a collimated structure is common in many stellar explosions.

    Research Briefing
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Reviews

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Research

  • Prolonged radio emissions above a sunspot, akin to those auroral emissions previously seen in the polar regions of planets and certain stars, have been detected using the Very Large Array. This detection could potentially provide support for an alternative mechanism for the origin of some stellar radio bursts.

    • Sijie Yu
    • Bin Chen
    • Marina Battaglia
    Article
  • The altered and thermally metamorphosed CY chondrites are shown to be the meteoritic analogue of asteroid Phaethon. This suggests that Phaethon’s activity is driven by gas released from the decomposition of near-surficial material heated at perihelion, whereas the interior is kept relatively unaltered and hydrated.

    • Eric MacLennan
    • Mikael Granvik
    Article
  • Juno’s close flyby of Ganymede on 7 June 2021 allowed the infrared mapping spectrometer JIRAM to observe the surface at unprecedented spatial resolution. JIRAM’s detailed spectroscopic characterization reveals past extensive aqueous alteration on the moon, possibly together with hydrothermal activity.

    • Federico Tosi
    • Alessandro Mura
    • Diego Turrini
    Article
  • Chemical disequilibrium is a known biosignature, and it is important to determine the conditions for its remote detection. A thermodynamical model coupled with atmospheric retrieval shows that a disequilibrium can be inferred for a Proterozoic Earth-like exoplanet in reflected light at a high O2/CH4 abundance case and signal-to-noise ratio of 50.

    • Amber V. Young
    • Tyler D. Robinson
    • James D. Windsor

    Collection:

    Article Open Access
  • A rare perfect alignment between two galaxies in the young Universe has been captured by the James Webb Space Telescope. The further (z ≈ 3) galaxy is curved into an Einstein ring due to the bending of space around the nearer (z ≈ 2) galaxy, which is massive and compact—representative of the pristine core of a present-day galaxy.

    • Pieter van Dokkum
    • Gabriel Brammer
    • Charlie Conroy
    Article Open Access
  • Synchrotron and inverse-Compton emission provide evidence for a reverse-shock origin of the high-energy emission from a gamma-ray burst, GRB 180720B. The polarization of the optical emission originating from the reverse shock suggests a turbulent shock that is amplified by the magnetic field in the relativistic ejecta.

    • Makoto Arimoto
    • Katsuaki Asano
    • Soebur Razzaque
    Article
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Amendments & Corrections

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