095.7332111 segreteria.direzione.oact@inaf.it | inafoacatania@pcert.postecert.it
  • Facebook
  • Twitter
  • RSS
  • Facebook
  • Twitter
  • RSS
Osservatorio Astrofisico di Catania
  • Home
  • Italiano
  • About us
    • Director
    • Structure Council
    • Personnel
    • Structures
      • “A. Riccò” (Catania)
      • “M. G. Fracastoro” (SLN)
    • Facilities
      • Laboratories
        • CASP
        • COLD
        • LASp
      • serra la nave observing station
      • Catania Solar Observations
      • library
      • Weather
        • Catania
        • Serra La Nave
    • Organizational Structure
    • Security
      • Safety at work
      • Covid-19
    • History
      • OACt History
      • List of Directors
      • Historical heritage museum (in progress)
  • Research
    • Research activities
    • Projects
    • Scientific publications
Select Page
First eclipse binary system discovered in NGC 2232

First eclipse binary system discovered in NGC 2232

by Daniela Sicilia | Aug 1, 2023 | Paper, Stellar Formation and Evolution

By combining the photometry of the TESS space telescope with the high-resolution spectroscopy of HARPS-N (TNG), a team of researchers, led by Antonio Frasca of the Osservatorio Astrofisico di Catania, has discovered a low-mass eclipsing binary system, the first in the...
Cheops shows scorching exoplanet acts like a mirror

Cheops shows scorching exoplanet acts like a mirror

by Daniela Sicilia | Jul 11, 2023 | Cheops, Exoplanets and Astrobiology, paper, Projects, RSN2

Data from ESA’s exoplanet mission Cheops has led to the surprising revelation that an ultra-hot exoplanet that orbits its host star in less than a day is covered by reflective clouds of metal, making it the shiniest exoplanet ever found.

Solar Orbiter crosses the Earth-Sun line as it heads for the Sun

Solar Orbiter crosses the Earth-Sun line as it heads for the Sun

by Daniela Sicilia | Mar 8, 2022 | Projects, RSN3, Solar Orbiter, Sun

The ESA/NASA Solar Orbiter spacecraft is speeding towards its historic first close pass of the Sun. On 14 March, the spacecraft will pass the orbit of Mercury, the scorched inner planet of our Solar System, and on 26 March it will reach closest approach to the Sun.

Recent Posts

  • Turbulence in the Sun’s corona
  • Juice rerouted to Venus in world’s first lunar-Earth flyby
  • Most massive stellar black hole in our galaxy found
  • Tiniest “starquakes” ever detected
  • First ‘glory’ on hellish distant world?

Tags

adaptive optics Ariel asteroseismology auroras Bh3 camera CCD detectors CHEOPS corona eclipse Elt ESA ESO Etna exoplanet exoplanets flare GAIA Gravity Inaf James Webb magnetic field MeerKat Mercury Milky Way perihelion planetary system planet formation Plato radio satellite Serra La Nave SoHO Solar Orbiter solar wind space weather Spitzer stellar oscillations Sun sunspots telescopes TESS turbulence ultra-hot Jupiter VLT

Meta

  • Log in
  • Entries feed
  • Comments feed
  • WordPress.org
  • Facebook
  • Twitter
  • RSS
INAF Osservatorio Astrofisico di Catania - C.F.: 97220210583 - Partita IVA: 06895721006                 Accessibilità