Barnaba Oriani | |
|---|---|
 | |
| Born | 17 July 1752 Garegnano, Milan, Duchy of Milan |
| Died | 12 November 1832 (aged 80) Milan, Kingdom of Lombardy–Venetia |
| Nationality | Italian |
| Occupations |
|
| Known for | detailed research of the planet Uranus |
| Parent(s) | Giorgio Oriani and Margherita Oriani (née Galli) |
| Scientific career | |
| Fields | astronomy |
| Institutions | Brera Astronomical Observatory |
Barnaba Oriani FRS FRSE (17 July 1752 – 12 November 1832) was an Italian priest, geodesist, astronomer and scientist.
Oriani was born in Garegnano (now part of Milan), the son of a mason,[1] and died in Milan.[2]
After getting his elementary education in Garegnano, he went on to study at the College of San Alessandro in Milan, under the tutelage and with the support of the Order of Barnabites,[3][4] which he later joined. After completing his studies in the humanities, physical and mathematical sciences, philosophy, and theology, he was ordained a priest in 1775.[2]
When Napoleon I established the Republic of Lombardy, Oriani refused to swear an oath against the monarchy, and the new republican government modified the oath of allegiance on his behalf. He was retained in his position at the observatory and was made president of the commission appointed to regulate the new system of weights and measures.[2]
When the republic became a Napoleonic kingdom, Oriani was awarded the Iron Crown and the Legion of Honour, was made a count and senator, and was appointed to measure the arc of the meridian between the zeniths of Rimini and Rome.[2]
Oriani was a devoted friend of the Theatine monk Giuseppe Piazzi, the discoverer of Ceres. Oriani and Piazzi worked together for thirty-seven years, cooperating on many astronomical observations.[2]
Given his strong interest in astronomy, Oriani was appointed on the staff of the Observatory of Brera in Milan in 1776, becoming assistant astronomer in 1778 and director in 1802. In 1778 he began publishing various in-depth dissertations on astronomical objects, the Effemeridi di Milano (Ephemerides of Milan).[2]
A very capable astronomer, Oriani's work began to attract considerable attention.[2] His research in the areas of astronomic refraction, the obliquity of the ecliptic, and orbital theory were of considerable noteworthiness in themselves; but his greatest achievement was his detailed research of the planet Uranus, which had been discovered by Sir William Herschel in 1781. Oriani devoted significant time to observations of Uranus, calculating its orbital properties which he published as a booklet of tables in 1793.[5]
After others had shown that Uranus was not on a parabolic orbit but rather in a roughly circular orbit, he calculated the orbit in 1783. In 1789, Oriani improved his calculations by accounting for the gravitational effects of Jupiter and Saturn.[3]
In addition to his continual contributions to the Effemeridi, he published a series of memoirs on spherical trigonometry: the Memorie dell' Istituto Italiano, 1806–10, and the Istruzione suelle misure e sui pesi, 1831.[2]
For his work in astronomy, Oriani was honoured by naming asteroid 4540 "Oriani". This asteroid had been discovered at the Osservatorio San Vittore in Bologna, Italy on 6 November 1988.[3]
In De refractionibus astronomicis,[6] Oriani showed that astronomical refraction could be expanded as a series of odd powers of (tan Z), where Z is the observed zenith distance. Such a series had previously been derived by J. H. Lambert, who dropped all but the first term. However, Oriani investigated the higher terms, and he found that neither of the first two terms depended on the structure of the atmosphere.
The series expansion he obtained was effective at up to 85 degrees from the zenith. Unlike previous approximations, however, Oriani's two-term expression did not depend on a hypothesis regarding atmospheric temperature or air density in relation to altitude. Thus, the effects of atmospheric curvature are only dependent upon the temperature and pressure at the location of the observer.
Oriani's theorem explains why Cassini's uniform-density model works well except near the horizon—the atmospheric refraction from the zenith to a zenith distance of 70° is not dependent on the details of the distribution of the gas.[7]
