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Comet De Vico
de Vico is the name of several comets discovered by Father Francesco de Vico, a Jesuit , image = Ihs-logo.svg , image_size = 175px , caption = ChristogramOfficial seal of the Jesuits , abbreviation = SJ , nickname = Jesuits , formation = , founders ... priest. See also * 54P/de Vico-Swift-NEAT, discovered 1844 August 23 * 122P/de Vico, discovered 1846 February 20 * C/1845 D1 (de Vico) * C/1846 B1 (de Vico) * C/1846 O1 (de Vico-Hind) * C/1846 S1 (de Vico) References NASA JPL database of comet orbital elements Comets 1840s in science {{comet-stub ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Francesco De Vico
Father Francesco de Vico (also known as de Vigo, De Vico and even DeVico; 19 May 1805 in Macerata – 15 November 1848 in London) was an Italian astronomer and a Jesuit priest. Biography He was educated at the college of Urbino, and became in 1835 assistant superintendent, and in 1839 director of the Vatican Observatory. The Revolutions of 1848 in the Italian states cut short his observing career, as he was forced into exile, touring Paris, London, and the United States, where he was received by the President. He was pleased with his reception in the U.S. and wished to settle there at Georgetown College, but first returned to Europe to try to recruit some colleagues to join him and purchase instruments for an observatory to be erected under his direction in New York. Unfortunately, worn out from the travel, he died in London in November of that same year Work He found a remarkable number of comets in a relatively short time, including periodic comets 54P/de Vico-Swift-NEAT and 1 ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Jesuit
, image = Ihs-logo.svg , image_size = 175px , caption = ChristogramOfficial seal of the Jesuits , abbreviation = SJ , nickname = Jesuits , formation = , founders = , founding_location = , type = Order of clerics regular of pontifical right (for men) , headquarters = Generalate:Borgo S. Spirito 4, 00195 Roma-Prati, Italy , coords = , region_served = Worldwide , num_members = 14,839 members (includes 10,721 priests) as of 2020 , leader_title = Motto , leader_name = la, Ad Majorem Dei GloriamEnglish: ''For the Greater Glory of God'' , leader_title2 = Superior General , leader_name2 = Fr. Arturo Sosa, SJ , leader_title3 = Patron saints , leader_name3 = , leader_title4 = Ministry , leader_name4 = Missionary, educational, literary works , main_organ = La Civiltà Cattolica ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
122P/de Vico
122P/de Vico (provisional designation: 1846 D1) is a periodic comet with an orbital period of 74 years. It fits the classical definition of a Halley-type comet with (20 years < < 200 years). It was discovered by in on February 20, 1846. During the 1846 apparition the comet reached a magnitude of 5 in mid March and was last observed in May. Its orbit was found to be elliptical and orbital calculations indicated that it would return between 1919 and 1925, however the comet wasn't detected. It was recovered on 17 September 1995 by the Japanese ast ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Comets
A comet is an icy, small Solar System body that, when passing close to the Sun, warms and begins to release gases, a process that is called outgassing. This produces a visible atmosphere or coma, and sometimes also a tail. These phenomena are due to the effects of solar radiation and the solar wind acting upon the nucleus of the comet. Comet nuclei range from a few hundred meters to tens of kilometers across and are composed of loose collections of ice, dust, and small rocky particles. The coma may be up to 15 times Earth's diameter, while the tail may stretch beyond one astronomical unit. If sufficiently bright, a comet may be seen from Earth without the aid of a telescope and may subtend an arc of 30° (60 Moons) across the sky. Comets have been observed and recorded since ancient times by many cultures and religions. Comets usually have highly eccentric elliptical orbits, and they have a wide range of orbital periods, ranging from several years to potentially several milli ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
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