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 1–7 of 7 results
Advanced filters: Author: Giovanna Tinetti Clear advanced filters
  • A report of recent observations of the close-in extrasolar giant planet (hot Jupiter) HD 189733b taken during the transit, where the planet passed in front of its parent star. Absorption by water vapour is the most likely cause of the wavelength-dependent variations in the effective radius of the planet.

    • Giovanna Tinetti
    • Alfred Vidal-Madjar
    • Franck Selsis
    Research
    Nature
    Volume: 448, P: 169-171
  • Water, carbon monoxide and methane are anticipated to be the main molecules (other than hydrogen) in the atmosphere of extrasolar planets. This paper reports a near-infrared transmission spectrum of the planet HD 189733b that shows the presence of methane and water, however, carbon monoxide is not seen.

    • Mark R. Swain
    • Gautam Vasisht
    • Giovanna Tinetti
    Research
    Nature
    Volume: 452, P: 329-331
  • Infrared spectroscopy can probe the conditions and compositions of exoplanet atmospheres. Previous results relied on space-based telescopes that do not provide spectroscopic capability in the 2.4–5.2 μm spectral region. Here, ground-based observations of the dayside emission spectrum for HD 189733b are reported between 2.0–2.4 μm and 3.1–4.1 μm; an unexpected feature at around 3.25 μm is found that is difficult to explain with models that assume local thermodynamic equilibrium conditions, and is assigned to methane.

    • Mark R. Swain
    • Pieter Deroo
    • Thomas Henning
    Research
    Nature
    Volume: 463, P: 637-639
  • High-performance scientific satellites are currently the exclusive domain of government-funded agencies. The team behind the Twinkle Space Mission is developing a new class of small and sustainable science satellites that leverages recent innovations in the commercial space sector.

    • Richard Archer
    • Marcell Tessenyi
    • Ben Wilcock
    Comments & Opinion
    Nature Astronomy
    Volume: 4, P: 1017-1018
  • K2-18 b is a planet with a mass around eight times that of the Earth that lies within the standard habitable zone of its star. Hubble spectra show the presence of an atmosphere around K2-18 b containing significant amounts of water vapour (up to a few tens of per cent, depending on the spectral model), but also a non-negligible amount of H2–He.

    • Angelos Tsiaras
    • Ingo P. Waldmann
    • Sergey N. Yurchenko
    Research
    Nature Astronomy
    Volume: 3, P: 1086-1091
  • The number of small satellites has grown hugely in the past decade, from tens of satellites per year in the mid-2010s to a projection of tens of thousands in orbit by the mid-2020s. This presents both problems and opportunities for observational astronomy. Small satellites offer complementary cost-effective capabilities to both ground-based astronomy and larger space missions. Compared with ground-based astronomy, these advantages are not just in the accessibility of wavelength ranges where the Earth’s atmosphere is opaque, but also in stable, high-precision photometry, long-term monitoring and improved areal coverage. Astronomy has a long history of new observational parameter spaces leading to major discoveries. Here we discuss the potential for small satellites to explore new parameter spaces in astrophysics, drawing on examples from current and proposed missions, and spanning a wide range of science goals from binary stars, exoplanets and Solar System science to the early Universe and fundamental physics.

    • Stephen Serjeant
    • Martin Elvis
    • Giovanna Tinetti
    Reviews
    Nature Astronomy
    Volume: 4, P: 1031-1038