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Letters On Sunspots
'' Letters on Sunspots'' (''Istoria e Dimostrazioni intorno alle Macchie Solari'') was a pamphlet written by Galileo Galilei in 1612 and published in Rome by the Accademia dei Lincei in 1613. In it, Galileo outlined his recent observation of dark spots on the face of the Sun. His claims were significant in undermining the traditional Aristotelian view that the Sun was both unflawed and unmoving. ''The Letters on Sunspots'' was a continuation of ''Sidereus Nuncius,'' Galileo's first work where he publicly declared that he believed that the Copernican system was correct. Previous observations of sunspots Galileo was not the first person to observe sunspots. The earliest apparent reference to them appears in the I Ching of ancient China, while the earliest recorded observation is also Chinese, dating to 364 BC. Around the same time, the first European mention of sunspots is found, by Theophrastus. There were reports from IslamicJ.M. Vaquero, M. Vázquez, The Sun Recorded Throug ...
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Galileo Macchie Solari
Galileo di Vincenzo Bonaiuti de' Galilei (15 February 1564 – 8 January 1642), commonly referred to as Galileo Galilei ( , , ) or mononymously as Galileo, was an Italian astronomer, physicist and engineer, sometimes described as a polymath. He was born in the city of Pisa, then part of the Duchy of Florence. Galileo has been called the father of observational astronomy, modern-era classical physics, the scientific method, and modern science. Galileo studied speed and velocity, gravity and free fall, the principle of relativity, inertia, projectile motion and also worked in applied science and technology, describing the properties of the pendulum and "hydrostatic balances". He was one of the earliest Renaissance developers of the thermoscope and the inventor of various sector (instrument), military compasses. With an improved telescope he built, he observed the stars of the Milky Way, the phases of Venus, the Galilean moons, four largest satellites of Jupiter, Saturn's r ...
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Transit Of Venus
A transit of Venus takes place when Venus passes directly between the Sun and the Earth (or any other superior planet), becoming visible against (and hence obscuring a small portion of) the solar disk. During a transit, Venus is visible as a small black circle moving across the face of the Sun. Transits of Venus reoccur periodically. A pair of transits takes place eight years apart in December (Gregorian calendar) followed by a gap of 121.5 years, before another pair occurs eight years apart in June, followed by another gap, of 105.5 years. The dates advance by about two days per 243-year cycle. The periodicity is a reflection of the fact that the orbital periods of Earth and Venus are close to 8:13 and 243:395 commensurabilities. The last pairs of transits occurred on 8 June 2004 and 5–6 June 2012. The next pair of transits will occur on 10–11 December 2117 and 8 December 2125. Transits of Venus were in the past used to determine the size of the Solar System. The ...
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Siderius Nuncius
''Sidereus Nuncius'' (usually ''Sidereal Messenger'', also ''Starry Messenger'' or ''Sidereal Message'') is a short astronomical treatise (or ''pamphlet'') published in Neo-Latin by Galileo Galilei on March 13, 1610. It was the first published scientific work based on observations made through a telescope, and it contains the results of Galileo's early observations of the imperfect and mountainous Moon, of hundreds of stars not visible to the naked eye in the Milky Way and in certain constellations, and of the Medicean Stars (later Galilean moons) that appeared to be circling Jupiter.Raphael, Renée. ''Sidereus nuncius; or, A Sidereal Message, by Galileo Galilei''. Isis, Vol. 101, No. 3 (September 2010), pp. 644-645. Published by: The University of Chicago Press on behalf of The History of Science Society. The Latin word ''nuncius'' was typically used during this time period to denote ''messenger''; however, it was also (though less frequently) rendered as ''message''. Though t ...
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Galilean Moons
The Galilean moons (), or Galilean satellites, are the four largest moons of Jupiter. They are, in descending-size order, Ganymede (moon), Ganymede, Callisto (moon), Callisto, Io (moon), Io, and Europa (moon), Europa. They are the most apparent magnitude, readily visible Solar System objects after Saturn, the dimmest of the classical planets; though their closeness to bright Jupiter makes naked-eye observation very difficult, they are readily seen with common binoculars, even under night sky Bortle scale, conditions of high light pollution. The invention of the telescope allowed astronomers to discover the moons in 1610. Through this, they became the first Timeline of discovery of Solar System planets and their moons, Solar System objects discovered since humans have started tracking the classical planets, and the first objects to be found to orbit any planet beyond Earth. They are planetary-mass moons and among the List of Solar System objects by size, largest objects in the Sola ...
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Roman Curia
The Roman Curia () comprises the administrative institutions of the Holy See and the central body through which the affairs of the Catholic Church are conducted. The Roman Curia is the institution of which the Roman Pontiff ordinarily makes use in the exercise of his supreme pastoral office and universal mission in the world: thus curialism refers traditionally to an emphasis on the supreme authority of the Holy See within the Catholic Church. It is at the service of the Pope and Bishops in the Catholic Church, bishops, fulfilling their function with an Gospel, evangelical spirit, working for the good and at the service of Communion of saints, communion, unity and edification of the Universal Church and attending to the demands of the world in which the Church is called to fulfill its duty and mission (''Praedicate evangelium'', article 1). The structure and organization of responsibilities within the Curia are at present regulated by the apostolic constitution issued by Pope F ...
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Dominican Order
The Order of Preachers (, abbreviated OP), commonly known as the Dominican Order, is a Catholic Church, Catholic mendicant order of pontifical right that was founded in France by a Castilians, Castilian priest named Saint Dominic, Dominic de Guzmán. It was approved by Pope Honorius III via the papal bull on 22 December 1216. Members of the order, who are referred to as Dominicans, generally display the letters ''OP'' after their names, standing for , meaning 'of the Order of Preachers'. Membership in the order includes friars, nuns, Religious sister (Catholic), active sisters, and Laity, lay or secular Dominicans (formerly known as Third Order of Saint Dominic, tertiaries). More recently, there have been a growing number of associates of the religious sisters who are unrelated to the tertiaries. Founded to preach the The gospel, gospel and to oppose heresy, the teaching activity of the order and its scholastic organisation placed it at the forefront of the intellectual life of ...
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Roman Inquisition
The Roman Inquisition, formally , was a system of partisan tribunals developed by the Holy See of the Catholic Church, during the second half of the 16th century, responsible for prosecuting individuals accused of a wide array of crimes according to Catholic law and doctrine, relating to Catholic religious life or alternative religious or secular beliefs. It was established in 1542 by the leader of the Catholic Church, Pope Paul III. In the period after the Medieval Inquisition, it was one of three different manifestations of the wider Catholic Inquisition, the other two being the Spanish Inquisition and Portuguese Inquisition. Function and functioning The main function of the institution was to maintain and implement papal bulls and other church rulings, in addition to their function of administering legalistic ramifications upon deviants of Catholic orthodoxy within states that cooperated with the pope and ostensibly exhibiting proper procedure to Catholic states in the proc ...
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Angelo De Filiis
Angelo is an Italian masculine given name and surname meaning "angel", or "messenger". People People with the given name *Angelo Abenante (1927–2024), Italian trade unionist and politician *Angelo Accardi, Italian visual artist *Angelo Accattino (born 1966), Italian prelate of the Catholic Church * Angelo Acciaioli, multiple people *Angelo Acerbi (born 1925), Catholic archbishop * Angelo Achini or Angiolo Achini (1850–1930), Italian painter *Angelo Acosta (born 2001), Filipino rapper *Angelo Agostini (1843–1910), illustrator, journalist and founder of several publications, and although born in Italy, is considered the first Brazilian cartoonist *Angelo Agrizzi, South African businessman and whistleblower * Angelo Aimo (born 1964), Italian footballer *Angelo Albanesi (late 1765–1784), Italian engraver *Angelo Alessandri (born 1969), Italian politician *Angelo Alessio (born 1965), Italian football manager and player *Angelo Alistar (born 1975), Romanian footballer *Angelo A ...
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Federico Cesi
Federico Angelo Cesi (; 26 February 1585 – 1 August 1630) was an Italian scientist, naturalist, and founder of the Accademia dei Lincei. On his father's death in 1630, he became briefly lord of Acquasparta. Biography Federico Cesi was born to an aristocratic family highly connected in Rome and the Papal States. The family derives its name from Cesi, a little town near Rome. They had a close connection with the Catholic Church, Frederico's uncle Bartolomeo Cesi was a cardinal in the church, and most of their wealth came from that connection. Federico was the first of eleven legitimate male children and was born in Palazzo Cesi, in via della Maschera d'Oro, Rome, on 26 February 1585. His father was Federico, marchese di Monticelli (1562–1630) and his mother was Olimpia Orsini of Todi. In 1614 Cesi was married to Artemisia Colonna, the daughter of Francesco, Principe di Palestrina; she died two years later. In 1617 he married Isabella, cousin of Filippo Salviati, the ...
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Helioscope
A helioscope is an instrument used in observing the Sun and sunspots. The helioscope was first used by Benedetto Castelli (1578–1643) and refined by Galileo Galilei (1564–1642). The method involves projecting an image of the sun onto a white sheet of paper suspended in a darkened room with the use of a telescope. The first ''machina helioscopica'' or helioscope was designed by Christoph Scheiner (1575 –1650) to assist his sunspot observations. (Latin) In the context of modern astroparticle physics, the term ''helioscope'' can also refer to an experiment that seeks to observe hypothetical particles (such as the axion) produced inside the sun. Examples of such helioscope experiments searching for axions include the CERN Axion Solar Telescope and International Axion Observatory. See also *Solar telescope * Heliometer *Spectroheliograph The spectroheliograph is an instrument used in astronomy which captures a photography, photographic image of the Sun at a single waveleng ...
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