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  • In-person and online conferences each have their benefits, with hybrid conferences intended to blend the best of both worlds. But do hybrid conferences fulfil the promise? Fifteen attendees across three global conferences share their collective experiences.

    • Vanessa A. Moss
    • Lola Balaguer-Nuñez
    • Adam R. H. Stevens
    Comment
  • Gamma-ray bursts are linked to the most distant objects in the Universe, but detecting them is a rare event. With a dedicated near-infrared telescope to observe in tandem with the optical Vera Rubin Observatory, ten or so high-redshift (z ≳ 6) gamma-ray bursts could potentially be detected every year.

    • S. Campana
    • G. Ghirlanda
    • S. D. Vergani
    Comment
  • The past three decades have seen the number of known exoplanets grow by over three orders of magnitude. To mark the milestone, the Lead Scientist of the NASA Exoplanet Archive, Jessie Christiansen, looks at the history, the contents and the future of this community resource.

    • Jessie L. Christiansen
    Comment
  • Cultural astronomy reveals ways in which perception and culture have shaped the interpretation of the night sky.

    • Charles Kemp
    • Duane W. Hamacher
    • Simon J. Cropper
    Comment
  • Equitable and high-quality scientific education is essential for fighting social inequalities and misinformation. The CosmoAmautas project aims to address this need and use astronomy to contribute to an accessible and decentralized scientific education in Peru.

    • Gabriela Calistro Rivera
    • Daniella Bardalez Gagliuffi
    • Erika Torre Ramirez
    Comment
  • The combination of hydrogen and carbon dioxide in the ocean of Enceladus represents chemical energy that could support life — but should we expect to see any energy ‘left on the table’ if anything alive is actually there to use it?

    • Tori M. Hoehler
    Comment
  • There is an ongoing debate as to whether ultra-diffuse galaxies are regular dwarf galaxies with low star formation or massive ‘failed’ objects that quenched their star formation in the early Universe. Current evidence seems to support the former scenario.

    • Ignacio Trujillo
    Comment
  • The Milky Way, Andromeda and Centaurus A host flattened arrangements of satellite dwarf galaxies with correlated kinematics. The rarity of similar structures in cosmological simulations constitutes a major problem for the ΛCDM model, with no obvious solution in sight.

    • Marcel S. Pawlowski
    Comment
  • The existence of planes of satellites has been a cosmological surprise. However, evidence for stable, long-lived satellite planes is generally tenuous, and they are unexpected in all current models of galaxy formation.

    • Michael Boylan-Kolchin
    Comment
  • In the past 20 years, the discovery and characterization of the smallest galaxies have pushed the edges of observational endeavours and theoretical advancements alike, and they will continue to be at the forefront of this field for years to come.

    • Denija Crnojević
    • Burçin Mutlu-Pakdil
    Comment
  • Alongside its role in astronomical research, the newly commissioned 32-m radio telescope is being used as an outreach tool for astronomy education in Ghana. The observatory also serves as a facility for international postgraduate programmes.

    • R. Aworka
    • E. Proven-Adzri
    • E. Aggrey
    Comment
  • Averting the imminent climate crisis requires large reductions in greenhouse gas emissions within this decade. To provide a benchmark for reduction and to identify the main sources, we estimate the carbon footprint of astronomy research in the Netherlands over 2019.

    • Floris van der Tak
    • Leo Burtscher
    • Arno Schoenmakers
    Comment
  • Recent work has questioned whether nature can extract the rotational energy of a black hole via electromagnetic fields. Although we show that the Blandford–Znajek effect is sound, the deeper physics of the electric nature of black holes remains unresolved.

    • David Garofalo
    • Chandra B. Singh
    Comment
  • The question of the possibility of life beyond Earth, as framed by the Drake equation, can be quantified to show that habitable environments for life as we know it are commonplace in the Galaxy.

    • Stephen J. Mojzsis
    Comment
  • Without a proper accounting of known and unknown systematics and uncertainties, combining information across multiple surveys, wavelengths, and detectors may be risky. Realizing the true potential of multi-messenger and panchromatic astrophysics requires getting data integration right.

    • Joshua S. Speagle (沈佳士)
    • Gwendolyn M. Eadie
    Comment
  • Astronomers are used to advocating for (financial) support for their future endeavours, but how should they go about lobbying for support for issues such as the climate emergency? Join forces with those experienced in effecting policy change.

    • Andrew Williams
    Comment
  • Astronomers are trusted voices in the communication of science; our community should resist inundating people with facts and figures but use its advantage to encourage the public to listen to climate change experts and encourage the need for urgent cross-sectoral systemic change.

    • Alison Anderson
    • Gina Maffey
    Comment
  • When do we stop an ongoing science project to make room for something new? Decision-making is a complex process, ranging from budgetary considerations and tension between ongoing projects, to progress assessments and allowance for novel science developments.

    • Ofer Lahav
    • Joseph Silk
    Comment
  • The climate crisis is no longer a prediction for the future, it is happening here and now. Astronomers have realized that they need to become part of the solution and are working towards reducing their own carbon footprint as well as communicating an astronomical perspective.

    • Leonard Burtscher
    • Hannah Dalgleish
    • Michelle Willebrands
    Comment
  • The missing baryon problem may now be resolved, but the exact location and physical properties of the diffuse component remains unclear. This problem could be tractable, but requires a combination of new galaxy redshift surveys and new X-ray and radio facilities.

    • Simon Driver
    Comment