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Galileo and the Telescope - University of Virginia
http://galileoandeinstein.physics.virginia.edu/lectures/galtel.pdf
WEBGalileo’s first major astronomical discovery with the telescope was that the Moon’s surface is mountainous, and not a perfect sphere as had always been assumed (see his drawings in Sidereus Nuncius). He built a convincing case for the reality of the mountains by sketching the appearance of parts of the Moon’s surface at different times of ...
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Galileo's telescope
https://brunelleschi.imss.fi.it/esplora/cannocchiale/dswmedia/risorse/complete_texts.pdf
WEBThe eyepiece consists of a biconcave lens with focal length of around 50 mm, and the instrument thus represents a late example of the Galilean telescope. 8. Terrestrial telescope by Eustachio Divini, 1660-1670, Florence, Institute and Museum of the History of Science. Telescope made of seven cardboard sections.
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Galileo and the telescope – Explaining Science
https://explainingscience.org/2018/03/13/galileo-and-the-telescope/
WEBMar 13, 2018 · Galileo turned his telescope to the Milky Way and discovered that it consisted of a vast number of stars, each too faint to be seen individually with the naked eye. When viewed from Earth these stars are so … pdf
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Galileo and the Telescope - Vanderbilt University
https://www.vanderbilt.edu/olli/class-materials/Exploration_Of_Astronomy_Session3.pdf
WEBGalileo and the Telescope. First observed the heavens telescopically in 1609. Discovered four large moons around Jupiter, mountains and other terrain on the surface of the Moon, phases of Venus, etc. Also observed sunspots and MW. Much of this was evidence that we do not live in an unchanging geocentric universe.
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14. Galileo and the Telescope. - New York University
https://research.engineering.nyu.edu/~jbain/mms/lectures/14.GalileoTele.pdf
WEB14.GalileoTele.pptx. 14. Galileo and the Telescope. The Starry Messenger (Sidereus Nuncius) (1610) 1608. Dutch lens-makers Hans Lippershey and Jacob Metius apply independently for patents on a device for "seeing faraway things as though nearby". (Sacharias Janssen also in possession of device.) 3×-4× magnification.
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Galileo and the physics of motion - Northern Illinois University
http://www.nicadd.niu.edu/~macc/162/class_3b.pdf
WEBKepler’s Laws. Kepler’s Laws can all be derived from Newton’s laws of motion and force of gravity. gravity causes elliptical orbits where planet moves faster when closer to the Sun as force of gravity is larger there. Third Law actually D3 = (Mass(sun) and Mass(earth) ) x P2 D=distance from Sun and P=period.
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Galileo’s telescope: history, scientific analysis, and …
https://link.springer.com/content/pdf/10.1007/s10686-009-9142-0.pdf
WEBGalileo’s telescope: history, scientific analysis, and replicated observations. Giorgio Strano. Received: 28 October 2008 / Accepted: 6 January 2009 / Published online: 24 January 2009 Springer Science + Business Media B.V. 2009. Abstract. In the summer of 1609, Galileo Galilei started to improve upon the Dutch spyglass.
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Galileo’s Knowledge of Optics and the Functioning of the …
https://arxiv.org/pdf/1307.4963.pdf
WEBoptics of telescopes and that Galileo conceived a novel theoretical framework. In this paper we respond to the challenge of the received view and establish the knowledge of optics that Galileo had as it can be read off from the telescopes he constructed and the way he put them to use. While our previous work is hypothetical,
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History of the Telescope and Its Remarkable Contribution to …
https://link.springer.com/content/pdf/10.1007/978-3-030-98828-9_1.pdf
WEBToday, some four hundred years after Galileo, magnificent telescopes, such as the 2.4-m Hubble Space Telescope, the 6.5-m James Webb Space Telescope (JWST), and the twin 10-m Keck telescopes, allow astronomers to see objects at incred-ible distances.
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Teaching and Research: Galilean and Keplerian Telescopes
https://cdn.ymaws.com/hssonline.org/resource/resmgr/teaching/galileankepleriantelescopes.pdf
WEBThe Galilean Telescope: The telescope Galileo used was a refracting telescope. It consisted of two lenses, one converging (which causes parallel light from the sun to converge to a focal point) and one diverging (which causes parallel light to diverge from a focal point), located at the ends of a long tube as shown in the figure below. Image Here.
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