The Astronomical Observatory of Rome (Osservatorio Astronomico di Roma in Italian) is one of twelve Astronomical Observatories in Italy. The main site of the Observatory is Monte Porzio Catone. Part of the Istituto Nazionale di Astrofisica since 2002.
Monte Mario Monte Mario Observatory (IAU code 034), the "historical" Observatory of Rome, located at 84 via del Parco Mellini in the northwest part of the city, atop Monte Mario, since 2002 is only the administrative seat of the Istituto Nazionale di Astrofisica (INAF). Nevertheless, the Astronomical Observatory of Roma has the responsibility for the Astronomical Copernican Museum and the Solar Tower in Monte Mario.
Monte Porzio Catone Monte Porzio Catone is located approximately 20 kilometres southeast of Rome proper. The Astronomical Observatory of Rome (OAR) was established in 1938, inside the 19th-century Villa Mellini on the hill of Monte Mario in Rome. In the same period, a new Observatory was built in Monteporzio Catone, in order to host a large telescope. With the Second World War, this project failed. In 1948, the building of Monteporzio was assigned to the Astronomical Observatory of Roma. In 1965, a new observing station was built in Campo Imperatore (2200 metres above sea level), on the Gran Sasso mountain. In 2017, the management of this station was transferred to the newly-established Osservatorio D’Abruzzo. Since 1988, the researchers of the Astronomical Observatory of Rome have been carrying out their research activity in Monteporzio Catone. The seat of Monteporzio includes the main building (three floors), the guesthouse, two small hoses for the janitors, AstroLAB, LightLAB, and the Monteporzio Telescope (MPT). These three latter structures are entirely devoted to public outreach. A few areas inside the main building are also occasionally used for visitors, i.e. historical rooms, “Livio Gratton” conference room, the modern library inside the main dome. The total area occupied by the structure within the compound sum up to about 8,750 square metres. Together with the garden, it adds up to about 75,000 square metres. OAR is responsible for the management of the “Museo Astronomico e Copernicano” (Astronomical Copernican Museum – MAC), in the ground floor of Villa Mellini. MAC was established in 1873 by Arthur Wolynski, upon the basis of a Copernican collection, put together on the occasion of the fourth centenary of the birth of Copernicus. This collection was implemented over the years with scientific instruments and historical books belonging to the older Observatories in the centre of Rome, following the evolution of astronomical instruments, private donations, and public institutes. The Museum's collection includes, among other objects, 17th century eyepieces, 14th century telescopes, sextants for measuring the angular distance between stars, astrolabes and night dials (the oldest astrolabe dates back to the twelfth century). Moreover, there is a rich collection of armillary spheres, as well as sky and Earth globes, including Mercatore's and Cassini's. The old library contains about 4000 volumes, some of which are rare and precious. For instance, there is a fourteenth century manuscript code, which collects the main astronomical works of the time, 5 incunabula, over 270 “cinquecentine” (16th century books) and 450 “secentine” (17th century books). In particular, among books of ancient Astronomy, one could mention the first editions of Copernicus’ works, Ptolem's Almagestos, Sacrobosco's Sphaera, Hevel's Theatrum Cometarum, Scheiner's Rosa Ursina, and the first editions of Galilei's works. Scientific and Technological Activity OAR's scientific productivity is quite high among the 20 institutes belonging to INAF, as proved by ANVUR's National check and by Nature Index. For example, in the year between November 2016 and November 2017, OAR researchers have taken part in writing 160 articles in referees reviews, which have produced 1597 citations. From 2014 to 2017, the total number of articles is 430, with 7555 citations. The scientific activity covers all the research areas inside INAF. In the Eighties and Nineties, the scientific area which involved most researchers, and was therefore the most productive was Stellar Astrophysics, with a remarkable number of researchers who were active in the areas of Extra-galactic Astrophysics and Solar Astrophysics. Starting from the mid-Nineties, a number of researchers were recruited in the areas of Relativistic Astrophysics, and Astrophysics of the Solar System. Nowadays, the scientific areas which absorbs most young researchers are Extra-galactic Astrophysics and Cosmology. OAR researchers make use of most Earth and space infrastructures, from radio to gamma rays:
ALMA, NOEMA, JVLA VLT, LBT, TNG, HST Chandra, XMM, Nustar, Swift Fermi, Magic OAR Researchers are either PI or are involved in a number of Large Programs on VLT, LBT, Chandra, and XMM. Cutting-edge research is in the following areas: Extra-galactic Astrophysics and Cosmology –
Accelerated Evolution of the Universe, Dark Matter, Dark Energy The first stars, galaxies, black holes, re-ionization of the Universe Formatione and evolution of galaxies, and of their Active Galactic Nuclei (AGN) Discovery and characterization Physical processes, stellar formation, accretion upon black holes, feedback Semi-analytical Models Stellar Astrophysics –
Synthesis of stellar populations Stellar Clusters Galaxies and the Local Group The production of dust and stellar winds Models and observations of Supernovae Stellar Evolution and Astroseismology Stellar Formation and proto-stars The Sun and the Solar System –
The structure of the magnetic field in the solar atmosphere Research and characterization of minor bodies of the Solar System Relativistic Astrophysics –
Neutron Stars Anatomy of Magnetars X-ray pulsars Equation of state of neutron stars Gamma-Ray Burst, Physics and Astrophysics Multi-messenger Astrophysics (Gravitational waves and e electromagnetic signals) OAR takes part in a large number of technological projects, both on the ground and in the space:
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