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Showing 1–7 of 7 results
Advanced filters: Author: Michael Fausnaugh Clear advanced filters

  • The authors report on a temperate Earth-sized planet orbiting the cool M6 dwarf LP 791-18 with a radius of 1.03 ± 0.04 R⊕ and an equilibrium temperature of 300–400 K, with the permanent night side plausibly allowing for water condensation.

    • Merrin S. Peterson
    • Björn Benneke
    • Thomas Barclay
    Research
    Nature
    Volume: 617, P: 701-705

  • Observations of TOI-849b reveal a radius smaller than Neptune’s but a large mass of about 40 Earth masses, indicating that the planet is the remnant core of a gas giant.

    • David J. Armstrong
    • Théo A. Lopez
    • Zhuchang Zhan
    Research
    Nature
    Volume: 583, P: 39-42

  • Observations from the JWST of the second brightest GRB ever detected, GRB 230307A, indicate that it belongs to the class of long-duration GRBs resulting from compact object mergers, with the decay of lanthanides powering the longlasting optical and infrared emission.

    • Andrew J. Levan
    • Benjamin P. Gompertz
    • David Alexander Kann
    ResearchOpen Access
    Nature
    Volume: 626, P: 737-741

  • The report of a 10,000 solar mass black hole in a dwarf galaxy provides new clues about how supermassive black holes form and grow with their host galaxies.

    • Michael Fausnaugh
    News & Views
    Nature Astronomy
    Volume: 3, P: 694-695

  • The Transiting Exoplanet Survey Satellite (TESS) has identified a nearby, bright, quiescent M dwarf star that hosts two sub-Neptune-sized planets and one super-Earth-sized planet. The system is eminently suitable for follow-up studies of transit timing variations, radial velocity measurements and transmission spectroscopy.

    • Maximilian N. Günther
    • Francisco J. Pozuelos
    • Ian A. Waite
    Research
    Nature Astronomy
    Volume: 3, P: 1099-1108