Filter By:

Journal Check one or more journals to show results from those journals only.

Choose more journals

Article type Check one or more article types to show results from those article types only.
Subject Check one or more subjects to show results from those subjects only.
Date Choose a date option to show results from those dates only.

Custom date range

Clear all filters
Sort by:
Showing 1–6 of 6 results
Advanced filters: Author: Hannu Parviainen Clear advanced filters
  • A nine-year transit-timing campaign has measured the extremely low masses and densities of four large planets orbiting the young star V1298 Tau, which are now predicted to contract and form a typical compact super-Earth and sub-Neptune system.

    • John H. Livingston
    • Erik A. Petigura
    • Lorenzo Pino
    ResearchOpen Access
    Nature
    Volume: 649, P: 310-314
  • Analysis of data from multiple instruments reveals a giant exoplanet in orbit around the 0.2-solar-mass star TOI-6894. The existence of this exoplanetary system challenges assumptions about planet formation and it is an excellent target for atmospheric characterization.

    • Edward M. Bryant
    • Andrés Jordán
    • Sebastián Zúñiga-Fernández
    ResearchOpen Access
    Nature Astronomy
    Volume: 9, P: 1031-1044
  • Observations of a fast X-ray transient reveal that it is a gamma-ray-burst explosion from a very distant galaxy that emits light with the wavelength necessary to drive cosmic reionization, the last major phase change in the history of the Universe.

    • Andrew J. Levan
    • Peter G. Jonker
    • Tayyaba Zafar
    Research
    Nature Astronomy
    Volume: 9, P: 1375-1386
  • 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
  • A giant planet candidate roughly the size of Jupiter but more than 14 times as massive is observed by TESS and other instruments to be transiting the white dwarf star WD 1856+534.

    • Andrew Vanderburg
    • Saul A. Rappaport
    • Liang Yu
    Research
    Nature
    Volume: 585, P: 363-367