Astronomical Figures

Total Page:16

File Type:pdf, Size:1020Kb

Astronomical Figures Astronomical Figures 190 BC - 120 BC Hipparchus, Astronomer Mathematicians *Devised latitudes and longitudes and created the apparent magnitude scale by d ividing stars into categories according to their brightness (1-6). (It wasn’t until the 1850's that scientists saw the brightest objects in the sky as brighter than first magnitude, so the system now has a rating of zero and negative magnitudes.) In fact, Sirius, the brightest star has a magnitude of -1.46, as seen from Earth. *If the magnitude is higher (fainter) than 6, the naked eye can’t see it. 90 - 168 Ptolemy, Astronomer / Geographer Mathematicians *Wrote the first astronomical account now known as the Almagest (" Mathematical Treatise ") *Ptolemy used Hipparchus's system of epicycles and eccentric circles to explain his geocentric theory of the universe. He believed the planets and sun orbit around the earth. This system became known as the Ptolemaic system. 1473 - 1543 Copernicus, Earth moves around the Sun Christians *Formulated the heliocentric theory that the universe orbits around the sun. 1546 - 1601 Tycho Brahe Mathematicians *Designed and built instruments, he also calibrated them and checked their accuracy periodically. 1564 - 1642 Galileo Galilei, Father of Modern Science Mathematicians *Made improvements to the telescope and astronomical observations, such as the imperfect surface of the Moon, the Phases of Venus, the Moons of Jupiter, and sunspots of the Sun. 1571 - 1630 Johannes Kepler, Laws Planetary Motion Mathematicians *Three laws of planetary motion that bear his name published in 1609 and 1619). 1625 - 1712 Giovanni Cassini, Astronomer Scientists *Determined the obliquity of the ecliptic at 23 deg 29' and studied the effects. 1643 - 1727 Isaac Newton, Theory of Gravitation Alchemists *Worked on optics and gravitation 1656 - 1742 Edmond Halley, Astronomer Mathematicians *mapped out stars and is known because of Haley’s Comet. 1701 - 1744 Anders Celsius, Temperature Scale Inventors *In 1742, he divided the temperature scale of a mercury thermometer at 760mm mercury air pressure into 100 degrees, where 100 is the freezing point and 0 the boiling point of water. 1738 - 1822 Herschel, Discovered Uranus - 1781 Composers *discovered Uranus and infrared radiation. 1811 - 1877 Le Verrier, Co-discovery of Neptune Mathematicians *studied the causes of disturbances in the Solar System. His work led to improved knowledge of the masses of the planets, the scale of the Solar System, and the velocity. 1819 - 1892 John Adams, Discovered Neptune - 1845 Discoveries * predicted the existence of Neptune. 1889 - 1953 Edwin Hubble, Big Bang Theory Mathematicians * devised a classification system for the various galaxies he observed, sorting them by content, distance, shape, and brightness; it was then he noticed redshifts in the emission of light from the galaxies. 1894 - 1966 Lemaître, Proposed Big Bang Theory Christians *proposed what became known as the Big Bang theory. 1905 - 1973 Gerard Kuiper, Astronomer Scientists *considered the father of modern planetary science for his wide ranging studies of the solar system. *established the atmosphere of Saturn's moon, Titan, and discovered Saturn's moon, Miranda, and Neptune's Nereid. Kuiper's prediction of comets traveling near the orbit of Neptune, the Kuiper belt. .
Recommended publications
  • Its Founding and Early Years Ewen A. Whitaker
    The University of Arizona's LUNAR AND PLANETARY LABORATORY Its Founding and Early Years Ewen A. Whitaker Set in Varityper Times Roman and printed at the University of Arizona Printing-Reproductions Department Equal Employment Opportunity· Affirmative Action Employer CONTENTS THE PRE-TUCSON ERA Historical background ........................................ I Enter Gerard P. Kuiper ....................................... 2 The Moon enters the picture ................................... 3 A call for suggestions ......................................... 5 The Harold Urey affair ....................................... 6 Preliminaries for the Lunar Atlas ............................... 7 1957 - a dream begins to take shape ............................. 7 The shot that was seen (and heard) around the world ............... 8 Other irons in the fire ......................................... 9 Kuiper seeks full-time help for the Lunar Project .................. 9 1959 - the Lunar Project gathers momentum ..................... 11 A new factor in the Lunar Project LPL story ................... 12 The Air Force enters the lunar cartography business ............... 13 The Lunar Atlas published at last .............................. 14 Big problems with the Yerkes set-up ............................ : 6 The southwestern U.S. begins to beckon ........................ 17 "There is a tide in the affairs of men ..." ....................... 18 Preparing for the move ...................................... 23 THE TUCSON ERA The Lunar Project makes the transfer
    [Show full text]
  • History of Space-Based Infrared Astronomy and the Air Force Infrared Celestial Backgrounds Program
    AFRL-RV-HA-TR-2008-1039 History of Space-Based Infrared Astronomy and the Air Force Infrared Celestial Backgrounds Program S. D. Price 18 April 2008 Approved for Public Release: Distribution Unlimited AIR FORCE RESEARCH LABORATORY Space Vehicles Directorate 29 Randolph Rd. Hanscom AFB, MA 01731-3010 AFRL-RV-HA-TR-2008-1039 This Technical Report has been reviewed and is approved for publication. / signed / ____________________________ Robert A. Morris, Chief Battlespace Environment Division / signed / / signed / _________________ _______________________________ Stephan D. Price Paul Tracy, Acting Chief Author Battlespace Surveillance Innovation Center This report has been reviewed by the ESC Public Affairs Office (PA) and is releasable to the National Technical Information Service. Qualified requestors may obtain additional copies from the Defense Technical Information Center (DTIC). All others should apply to the National Technical Information Service (NTIS). If your address has changed, if you wish to be removed from the mailing list, of if the address is no longer employed by your organization, please notify AFRL/VSIM, 29 Randolph Rd., Hanscom AFB, MA 01731-3010. This will assist us in maintaining a current mailing list. Do not return copies of this report unless contractual obligations or notices on a specific document require that it be returned. Form Approved REPORT DOCUMENTATION PAGE OMB No. 0704-0188 The public reporting burden for this collection of information is estimated to average 1 hour per response, including the time for reviewing instructions, searching existing data sources, gathering and maintaining the data needed, and completing and reviewing the collection of information. Send comments regarding this burden estimate or any other aspect of this collection of information, including suggestions for reducing the burden, to Department of Defense, Washington Headquarters Services, Directorate for Information Operations and Reports (0704-0188), 1215 Jefferson Davis Highway, Suite 1204, Arlington, VA 22202-4302.
    [Show full text]
  • Astronomy Alphabet
    Astronomy Alphabet Educational video for children Teacher https://vimeo.com/77309599 & Learner Guide This guide gives background information about the astronomy topics mentioned in the video, provides questions and answers children may be curious about, and suggests topics for discussion. Alhazen A Alhazen, called the Father of Optics, performed NASA/Goddard/Lunar Reconnaissance Orbiter, Apollo 17 experiments over a thousand years ago Can you find Alhazen crater when you look at the Moon? to learn about how light travels and Why does the Moon look bigger near the behaves. He also studied astronomy, horizon? separated light into colors, and sought to Believe it or not, scientists still don’t know for sure why explain why the Moon looks bigger near we perceive the Moon to be larger when it lies near to the the horizon. horizon. Though photos of the Moon at different points in the sky show it to be the same size, we humans think we I’ve never heard of Abu Ali al-Hasan ibn al- see something quite different. Try this experiment yourself Hasan ibn al-Hatham (Alhazen). sometime! One possibility is that objects we see next to the Tell me more about him. Moon when it’s near to them give us the illusion that it’s We don’t know that much about Alhazen be- bigger, because of a sense of scale and reference. cause he lived so long ago, but we do know that he was born in Persia in 965. He wrote hundreds How many craters does the Moon have, and what of books on math and science and pioneered the are their names? scientific method of experimentation.
    [Show full text]
  • Titan a Moon with an Atmosphere
    TITAN A MOON WITH AN ATMOSPHERE Ashley Gilliam Earth 450 – Satellites of Jupiter and Saturn 4/29/13 SATURN HAS > 60 SATELLITES, WHY TITAN? Is the only satellite with a dense atmosphere Has a nitrogen-rich atmosphere resembles Earth’s Is the only world besides Earth with a liquid on its surface • Possible habitable world Based on its size… Titan " a planet in its o# $ght! R = 6371 km R = 2576 km R = 1737 km Ch$%iaan Huy&ns (1629-1695) DISCOVERY OF TITAN Around 1650, Huygens began building telescopes with his brother Constantijn On March 25, 1655 Huygens discovered Titan in an attempt to study Saturn’s rings Named the moon Saturni Luna (“Saturns Moon”) Not properly named until the mid-1800’s THE DISCOVERY OF TITAN’S ATMOSPHERE Not much more was learned about Titan until the early 20th century In 1903, Catalan astronomer José Comas Solà claimed to have observed limb darkening on Titan, which requires the presence of an atmosphere Gerard P. Kuiper (1905-1973) José Comas Solà (1868-1937) This was confirmed by Gerard Kuiper in 1944 Image Credit: Ralph Lorenz Voyager 1 Launched September 5, 1977 M"sions to Titan Pioneer 11 Launched April 6, 1973 Cassini-Huygens Images: NASA Launched October 15, 1997 Pioneer 11 Could not penetrate Titan’s Atmosphere! Image Credit: NASA Vo y a &r 1 Image Credit: NASA Vo y a &r 1 What did we learn about the Atmosphere? • Composition (N2, CH4, & H2) • Variation with latitude (homogeneously mixed) • Temperature profile Mesosphere • Pressure profile Stratosphere Troposphere Image Credit: Fulchignoni, et al., 2005 Image Credit: Conway et al.
    [Show full text]
  • SOFIA-NASA's Stratospheric Observatory for Infrared Astronomy
    SOFIA-NASA’s Stratospheric Observatory for Infrared Astronomy NASA’s SOFIA 747SP during an early check flight over the Texas countryside. ED07-0079-02 NASA is developing the Stratospheric Observa- Unparalleled astronomical science capabilities tory for Infrared Astronomy – or SOFIA – as a world-class airborne observatory that will comple- Once it begins operations in about 2010, ment the Hubble, Spitzer, Herschel and James SOFIA’S 2.5-meter (98.4-inch) diameter reflect- Webb space telescopes and major Earth-based ing telescope will provide astronomers with ac- telescopes. SOFIA features a German-built 98.4- cess to the visible, infrared and sub-millimeter inch (2.5 meter) diameter far-infrared telescope spectrum, with optimized performance in the weighing 20 tons mounted in the rear fuselage of mid-infrared to sub-millimeter range. During its a highly modified Boeing 747SP aircraft. It is one 20-year expected lifetime, SOFIA’s telescope of the premier space science programs of NASA’s will be capable of “Great Observatory”-class Science Mission Directorate. astronomical science. SOFIA is a joint program by NASA and DLR SOFIA will continue the legacy of prominent Deutsches Zentrum fur Luft- und Raumfahrt (Ger- planetary scientist Dr. Gerard Kuiper, who be- man Aerospace Center). Major aircraft modifica- gan airborne astronomy in 1966 with a 12-inch tions and installation of the telescope has been telescope aimed out a window of a converted carried out at L-3 Communications Integrated Convair 990 jetliner. His work led to the devel- Systems facility at Waco, Texas. Completion of opment of NASA’s Kuiper Airborne Observa- systems installation, integration and flight test tory, a modified C-141 aircraft incorporating operations are being conducted at NASA’s Dryden a 36-inch reflecting telescope that flew from Flight Research Center at Edwards Air Force Base, 1974 to 1995.
    [Show full text]
  • Flying Telescopes, "Mercury Magazine"
    FLYINGFLYING TELESCOPESTELESCOPES Following nearly four decades of bigger and better airborne observatories, NASA’s SOFIA mission will carry infrared astronomy to new heights. For nearly 40 years, astronomers This Boeing 747SP, shown during a 1998 by Sally Stephens have battled air turbulence, engine test flight, will house the SOFIA infrared vibrations, and complicated aerody- telescope. The painted dark rectangular area on the rear of the fuselage marks the namics of wind blowing past a hole in telescope’s location.This aircraft is named he airplane looks like any an airplane’s side to gain a view of the the Clipper Lindbergh. It was christened in other 747, until you notice the universe impossible to achieve from 1977 by Anne Morrow Lindbergh on the large, gaping hole in its left the ground. Airborne astronomy has 50th anniversary of her late husband’s solo side, just behind the wing. The shown scientists the secrets of star transatlantic flight. Courtesy of L3 Com- hole is no accident. It will give formation, planetary rings, and the munications, Integrated Systems. astronomers an unobstructed energetic cores of galaxies. view of the universe through a But why go to all the trouble? rays, which would otherwise damage T 2.5-meter telescope mounted Ground-based telescopes work well skin and other cells in our bodies. But inside the plane. When the airplane, for studying the sky in visible light. it’s bad when it comes to infrared nicknamed SOFIA, finally takes flight But Earth’s atmosphere blocks most light, also known as thermal radia- in 2004, it will become the latest in a other forms of light from reaching the tion or heat.
    [Show full text]
  • Outline Pluto's Surface
    • Last Homework before Exam (HW#4) is due Friday Outline at 11:50am. •Pluto – Different– planet or Kuiper belt object • Nighttime observing has 4 more nights. Check the • Asteroids webpage. – Near Earth • Meteoroid, Meteor, and Meteorites • 1st exam is October 10th– 1 week away! – Mostly from asteroids • Radioactivity– interlude •Comets • Justin will have an extra office hour Thursday (10/9) – Short term– Kuiper Belt before exam– 4:00 to 5:00pm. – Long Term– Oort Cloud • Meteor showers • I will have an extra office hour Wednesday (10/8) • Kuiper Belts Objects before exam– 10:30 to 11:30am. Oct 3, 2003 Astronomy 100 Fall 2003 Oct 3, 2003 Astronomy 100 Fall 2003 Earth – Pluto - Charon comparison Pluto’s Surface • http://www.solarviews.com/raw/pluto/vpluchar.mpg • The only planet not yet visited by a spacecraft • Largest range of albedo yet observed in Solar System • Dark areas – rock • Light areas – frost • Surface features > 500 km in size Smallest planet or Radius 0.19 Earth Surface gravity 0.055 Earth largest Kuiper belt Mass 0.002 Earth object. Coldest Distance from Sun 39.5 AU planet. Has biggest Eccentricity 0.249 moon relative to Tilt 118° itself and the Albedo 0.5 largest tilt of orbit Year 248.6 Earth years around Sun. Solar day 6.39 Earth days (retrograde) http://www.solarviews.com/cap/pluto/hstpluto.htm Oct 3, 2003 Astronomy 100 Fall 2003 Oct 3, 2003 Astronomy 100 Fall 2003 Pluto’s Atmosphere • Observed when Pluto occults background stars • Consists mostly of nitrogen (90%) and methane • Alternately freezes and sublimates as Pluto-Sun
    [Show full text]
  • Gerard Peter Kuiper
    NATIONAL ACADEMY OF SCIENCES G ERARD PETER K UIPER 1905—1973 A Biographical Memoir by D A L E P . CRUIKSHANK Any opinions expressed in this memoir are those of the author(s) and do not necessarily reflect the views of the National Academy of Sciences. Biographical Memoir COPYRIGHT 1993 NATIONAL ACADEMY OF SCIENCES WASHINGTON D.C. GERARD PETER KUIPER December 7, 1905-December 24, 1973 BY DALE P.CRUIKSHANK OW DID THE SUN and planets form in the cloud of gas H and dust called the solar nebula, and how does this genesis relate to the formation of other star systems? What is the nature of the atmospheres and the surfaces of the planets in the contemporary solar system, and what have been their evolutionary histories? These were the driv- ing intellectual questions that inspired Gerard Kuiper's life of observational study of stellar evolution, the properties of star systems, and the physics and chemistry of the Sun's family of planets. Gerard Peter Kuiper (originally Gerrit Pieter Kuiper) was born in The Netherlands in the municipality of Haringcarspel, now Harenkarspel, on December 7, 1905, son of Gerrit and Antje (de Vries) Kuiper. He died in Mexico City on December 24, 1973, while on a trip with his wife and his long-time friend and colleague, Fred Whipple. He was the first of four children; his sister, Augusta, was a teacher before marriage, and his brothers, Pieter and Nicolaas, were trained as engineers. Kuiper's father was a tailor. Young Kuiper was an outstanding grade school student, but for a high school education he was obliged to leave his small town and go to Haarlem to a special institution that would lead him to a career as a primary school teacher.
    [Show full text]
  • Next Stop: Uranus
    www.astrosociety.org/uitc No. 4 - Winter 1985-86 © 1986, Astronomical Society of the Pacific, 390 Ashton Avenue, San Francisco, CA 94112 Next Stop: Uranus On January 24, 1986. the aging but still active Voyager 2 spacecraft will become the first mission to fly by the seventh planet in our solar system. a giant, bluish-green, and often puzzling world called Uranus. Mission scientists predict that we will learn more about this distant planet in the six hours of closest encounter than we have in the roughly 200 years since Uranus was discovered. In this issue of The Universe in the Classroom, we summarize our current knowledge of the complex Uranus system and provide some background to help you evaluate and explain the Voyager results to your classes. History Uranus was the first planet to be discovered that was not known to the ancients. It was found on March 13, 1781 by an amateur astronomer (and professional musician) named William Herschel, using a homemade 6.2-inch telescope. At first Herschel thought he had merely discovered a new comet, but it soon became apparent that the new object behaved like a planet. After some debate it was named Uranus, after the god in Greek mythology who most closely personified the heavens. (Uranus was the father of the Titans and thus grandfather of Jupiter.) As a result of his pioneering find, Herschel received a life-long stipend from the king of England and was able to continue building larger and larger telescopes and making a host of important discoveries. Among these was his spotting of two of Uranus's moons, Titania and Oberon, in 1787.
    [Show full text]
  • Kuiper Belt and Oort Cloud
    National Aeronautics and Space Administration Typical KBO Orbit Kuiper Belt Pluto’s Orbit Oort Cloud Eris Kuiper Belt and Oort Cloud www.nasa.gov In 1950, Dutch astronomer Jan Oort proposed that certain One of the most unusual KBOs is Haumea, part of a collisional SIGNIFICANT DATES comets come from a vast, extremely distant, spherical shell of family orbiting the Sun, the first found in the Kuiper Belt. The 1943 — Astronomer Kenneth Edgeworth suggests that a reser- icy bodies surrounding the solar system. This giant swarm of parent body, Haumea, apparently collided with another object voir of comets and larger bodies resides beyond the planets. objects is now named the Oort Cloud, occupying space at a that was roughly half its size. The impact blasted large icy 1950 — Astronomer Jan Oort theorizes that a vast population distance between 5,000 and 100,000 astronomical units. (One chunks away and sent Haumea reeling, causing it to spin end- of comets may exist in a huge cloud on the distant edges of our astronomical unit, or AU, is the mean distance of Earth from the over-end every four hours. It spins so fast that it has pulled itself solar system. Sun: about 150 million kilometers or 93 million miles.) The outer into the shape of a squashed American football. Haumea and 1951 — Astronomer Gerard Kuiper predicts the existence of a extent of the Oort Cloud is considered to be the “edge” of our two small moons — Hi’iaka and Namaka — make up the family. belt of icy objects just beyond the orbit of Neptune.
    [Show full text]
  • Kuiper Belt and Oort Cloud Lithograph
    National Aeronautics and Space Administration Typical KBO Orbit Kuiper Belt Pluto’s Orbit Oort Cloud Eris Outer Solar System Kuiper Belt and Oort Cloud www.nasa.gov In 1930, soon after the discovery of Pluto, astronomer Fred- more comets. Because KBOs are so distant, their sizes are dif- While no spacecraft has yet traveled to the Kuiper Belt, NASA’s erick C. Leonard suggested that Pluto was but one of many ficult to measure. The calculated diameter of a KBO depends on New Horizons spacecraft, which is scheduled to arrive at Pluto “ultra-Neptunian” or “trans-Neptunian” small bodies. In 1943, assumptions about how brightness relates to size. With infrared in 2015, plans to study other KBOs after the Pluto mission is astronomer Kenneth Edgeworth hypothesized that many small, observations by the Spitzer Space Telescope, most of the largest complete. icy bodies exist in a disc in the region beyond Neptune, having KBOs have known sizes. condensed from widely spaced ancient material, and that from SIGNIFICANT DATES One of the most unusual KBOs is Haumea, part of a collisional time to time one of them visits the inner solar system. Eight family orbiting the Sun, the first found in the Kuiper Belt. The 1943 — Astronomer Kenneth Edgeworth suggests that a reser- years later, Gerard Kuiper proposed the existence of such a parent body, Haumea, apparently collided with another object voir of comets and larger bodies resides beyond the planets. disc, which formed early in the solar system’s evolution. In 1992, that was roughly half its size. The impact blasted large icy 1950 — Astronomer Jan Oort theorizes that a vast population of astronomers detected a faint speck of light from an object about chunks away and sent Haumea reeling, causing it to spin end- comets may exist in a huge cloud surrounding our solar system.
    [Show full text]
  • From Planet X to Planet Nine
    From Planet X to Planet Nine Nuno Peixinho Café com Física 2016 The Triumph of Celestial Mechanics Neptune Finding Neptune • Neptune was teh first planet to be discoverd by prediction. • 1781, Anders Johan Lexell saw that there were irregularities in Uranus´ orbit. • 1846, Urbain Le Verrier predicted the mass and location for the unknown planet that would explain such irregularities. • Johann Gottfried Galle and Heinrich Louis d’Arrest find it at the Observatory of Berlin on the same day (at night, of coutrse) they received the news: September 23rd, 1846. • John Couch Adams also had predicted Neptune and he has credit for that but… “Planet-X” Planet O, P, Q, R, S, T, and U • William Pickering is the most prolific postulator of undiscoverd planets. • From 1908 to 1932, Pickering proposed seven hypothetical planets: O, P, Q, R, S, T and U. ⇒ Planet S Proposed in 1928; given elements in 1931: a=48.3 AU, P=336 yr, M=5M, mag=15. ⇒ Planet O Proposed in 1908; given elements in 1928: a=35.2 AU, P=209 yr, M=0.5M, mag=12. Planet X • Persival Lowell was searching for his Planet X. • During 1906, using a 5-inch (13 cm) camera. • From 1914 to 1916, a 9-inch (23 cm) telescope. ⇒ Planet X Proposed in 1906; given elements in 1927: a=43 AU, P=282 yr, M=6.6M, mag=12-13. • Never found anything but… Lowell Observatory did photograph Pluto in March and April 1915!!! • He founded the Lowell Observatory as private. Pluto • Clyde Tombaugh, a farm boy who was an amateur astronomer, was hired in 1929.
    [Show full text]