12 Planets in Our Solar System?
Total Page:16
File Type:pdf, Size:1020Kb
Load more
Recommended publications
-
Demoting Pluto Presentation
WWhhaatt HHaappppeenneedd ttoo PPlluuttoo??!!!! Scale in the Solar System, New Discoveries, and the Nature of Science Mary L. Urquhart, Ph.D. Department of Science/Mathematics Education Marc Hairston, Ph.D. William B. Hanson Center for Space Sciences FFrroomm NNiinnee ttoo EEiigghhtt?? On August 24th Pluto was reclassified by the International Astronomical Union (IAU) as a “dwarf planet”. So what happens to “My Very Educated Mother Just Served Us Nine Pizzas”? OOffifficciiaall IAIAUU DDeefifinniittiioonn A planet: (a) is in orbit around the Sun, (b) has sufficient mass for its self-gravity to overcome rigid body forces so that it assumes a hydrostatic equilibrium (nearly round) shape, and (c) has cleared the neighborhood around its orbit. A dwarf planet must satisfy only the first two criteria. WWhhaatt iiss SScciieennccee?? National Science Education Standards (National Research Council, 1996) “…science reflects its history and is an ongoing, changing enterprise.” BBeeyyoonndd MMnneemmoonniiccss Science is “ not a collection of facts but an ongoing process, with continual revisions and refinements of concepts necessary in order to arrive at the best current views of the Universe.” - American Astronomical Society AA BBiitt ooff HHiiststoorryy • How have planets been historically defined? • Has a planet ever been demoted before? Planet (from Greek “planetes” meaning wanderer) This was the first definition of “planet” planet Latin English Spanish Italian French Sun Solis Sunday domingo domenica dimanche Moon Lunae Monday lunes lunedì lundi Mars Martis -
Galileo and the Telescope
Galileo and the Telescope A Discussion of Galileo Galilei and the Beginning of Modern Observational Astronomy ___________________________ Billy Teets, Ph.D. Acting Director and Outreach Astronomer, Vanderbilt University Dyer Observatory Tuesday, October 20, 2020 Image Credit: Giuseppe Bertini General Outline • Telescopes/Galileo’s Telescopes • Observations of the Moon • Observations of Jupiter • Observations of Other Planets • The Milky Way • Sunspots Brief History of the Telescope – Hans Lippershey • Dutch Spectacle Maker • Invention credited to Hans Lippershey (c. 1608 - refracting telescope) • Late 1608 – Dutch gov’t: “ a device by means of which all things at a very great distance can be seen as if they were nearby” • Is said he observed two children playing with lenses • Patent not awarded Image Source: Wikipedia Galileo and the Telescope • Created his own – 3x magnification. • Similar to what was peddled in Europe. • Learned magnification depended on the ratio of lens focal lengths. • Had to learn to grind his own lenses. Image Source: Britannica.com Image Source: Wikipedia Refracting Telescopes Bend Light Refracting Telescopes Chromatic Aberration Chromatic aberration limits ability to distinguish details Dealing with Chromatic Aberration - Stop Down Aperture Galileo used cardboard rings to limit aperture – Results were dimmer views but less chromatic aberration Galileo and the Telescope • Created his own (3x, 8-9x, 20x, etc.) • Noted by many for its military advantages August 1609 Galileo and the Telescope • First observed the -
Earth Venus Mercury the Sun Saturn Jupiter Uranus Mars
Mercury Diameter 1,391,000 km Diameter 4878 km Diameter 12,104 km Diameter 12,756 km Temperature 6000°C Temperature 427°C Temperature 482°C Temperature 22°C Speed 136 mph Speed 107,132 mph Speed 78,364 mph Speed 66,641 mph Mass 1,989,000 Mass 0.33 Mass 4.86 Mass 5.97 Year of Discovery N/A Year of Discovery Venus 1885 Year of Discovery N/A Year of Discovery N/A The Sun Mercury Earth Mercury is the closest planet to the sun, orbiting our star at an average distance of 57.9 million kilometres, taking 88 days to complete a trip around the sun. Mercury is also the smallest planet in our solar system. Mercury is the closest planet to the Sun, orbiting The Sun is the star at the centre of our Solar our star at an average distance of 57.9 million Venus is our neighbouring planet. It is Our home, some 4.5 billion years old. Life System. Its mass is approximately 330,000 times kilometres, taking 88 days to complete a trip impossible to state when Venus was appeared on the surface just 1 billion years heavier than our home planet and is 109 times around the sun. Mercury is also the smallest after creation, with human beings appearing wider. The Sun is the largest object in our Solar planet in our Solar System. discovered as it is visible with the just 200,000 years ago. System. naked eye. Diameter 6794 km Diameter 142,800 km Saturn Diameter 120,536 km Diameter 51,118 km Temperature -15°C Temperature -150°C Temperature -180°C Temperature -214°C Speed 53,980 mph Speed 29,216 mph Speed 21,565 mph Speed 15,234 mph Mass 0.64 Mass 1898 Mass 568 Mass 86.81 Mars Year of Discovery 1580 Year of Discovery 1610 Year of Discovery 700 BC Year of Discovery 1781 Jupiter Uranus The fourth planet from the Sun. -
Ices on Mercury: Chemistry of Volatiles in Permanently Cold Areas of Mercury’S North Polar Region
Icarus 281 (2017) 19–31 Contents lists available at ScienceDirect Icarus journal homepage: www.elsevier.com/locate/icarus Ices on Mercury: Chemistry of volatiles in permanently cold areas of Mercury’s north polar region ∗ M.L. Delitsky a, , D.A. Paige b, M.A. Siegler c, E.R. Harju b,f, D. Schriver b, R.E. Johnson d, P. Travnicek e a California Specialty Engineering, Pasadena, CA b Dept of Earth, Planetary and Space Sciences, University of California, Los Angeles, CA c Planetary Science Institute, Tucson, AZ d Dept of Engineering Physics, University of Virginia, Charlottesville, VA e Space Sciences Laboratory, University of California, Berkeley, CA f Pasadena City College, Pasadena, CA a r t i c l e i n f o a b s t r a c t Article history: Observations by the MESSENGER spacecraft during its flyby and orbital observations of Mercury in 2008– Received 3 January 2016 2015 indicated the presence of cold icy materials hiding in permanently-shadowed craters in Mercury’s Revised 29 July 2016 north polar region. These icy condensed volatiles are thought to be composed of water ice and frozen Accepted 2 August 2016 organics that can persist over long geologic timescales and evolve under the influence of the Mercury Available online 4 August 2016 space environment. Polar ices never see solar photons because at such high latitudes, sunlight cannot Keywords: reach over the crater rims. The craters maintain a permanently cold environment for the ices to persist. Mercury surface ices magnetospheres However, the magnetosphere will supply a beam of ions and electrons that can reach the frozen volatiles radiolysis and induce ice chemistry. -
Callisto: a Guide to the Origin of the Jupiter System
A PAPER SUBMITTED TO THE DECADAL SURVEY ON PLANETARY SCIENCE AND ASTROBIOLOGY Callisto: A Guide to the Origin of the Jupiter System David E Smith 617-803-3377 Department of Earth, Atmospheric and PLanetary Sciences Massachusetts Institute of Technology, Cambridge MA 02139 [email protected] Co-authors: Francis Nimmo, UCSC, [email protected] Krishan Khurana, UCLA, [email protected] Catherine L. Johnson, PSI, [email protected] Mark Wieczorek, OCA, Fr, [email protected] Maria T. Zuber, MIT, [email protected] Carol Paty, University of Oregon, [email protected] Antonio Genova, Univ Rome, It, [email protected] Erwan Mazarico, NASA GSFC, [email protected] Louise Prockter, LPI, [email protected] Gregory A. Neumann, NASA GSFC Emeritus, [email protected] John E. Connerney, Adnet Systems Inc., [email protected] Edward B. Bierhaus, LMCO, [email protected] Sander J. Goossens, UMBC, [email protected] MichaeL K. Barker, NASA GSFC, [email protected] Peter B. James, Baylor, [email protected] James Head, Brown, [email protected] Jason Soderblom, MIT, [email protected] July 14, 2020 Introduction Among the GaLiLean moons of Jupiter, it is outermost CaLListo that appears to most fulLy preserve the record of its ancient past. With a surface aLmost devoid of signs of internaL geologic activity, and hints from spacecraft data that its interior has an ocean whiLe being only partiaLLy differentiated, CaLListo is the most paradoxicaL of the giant rock-ice worlds. How can a body with such a primordiaL surface harbor an ocean? If the interior was warm enough to form an ocean, how could a mixed rock and ice interior remain stable? What do the striking differences between geologicaLLy unmodified CaLListo and its sibling moon Ganymede teLL us about the formation of the GaLiLean moons and the primordiaL conditions at the time of the formation of CaLListo and the accretion of giant planet systems? The answers can be provided by a CaLListo orbitaL mission. -
TAKE-HOME EXP. # 1 Naked-Eye Observations of Stars and Planets
TAKE-HOME EXP. # 1 Naked-Eye Observations of Stars and Planets Naked-eye observations of some of the brightest stars, constellations, and planets can help us locate our place in the universe. Such observations—plus our imaginations—allow us to actively participate in the movements of the universe. During the last few thousand years, what humans have said about the universe based on naked-eye observations of the night and day skies reveals the tentativeness of physical models based solely on sensory perception. Create, in your mind's eye, the fixed celestial sphere. See yourself standing on the Earth at Observer's the center of this sphere. As you make the zenith + star-pattern drawings of this experiment, your perception may argue that the entire sphere of fixed star patterns is moving around the Earth and you. To break that illusion, you probably have to consciously shift your frame of º reference—your mental viewpoint, in this 50 up from the horizon case— to a point far above the Earth. From South there you can watch the globe of Earth slowly Observer on local horizon plane rotate you , while the universe remains essentially stationary during your viewing It is you that turns slowly underneath a fixed and unchanging pattern of lights. Naked eye observations and imagination has led to constellation names like "Big Bear" or "Big Dipper". These names don't change anything physically —except, and very importantly, they aid humans' memory and use of star patterns. A. Overview This experiment involves going outside to a location where you can observe a simple pattern of stars, including at least 2, but preferably 3 or 4 stars. -
Bepicolombo - a Mission to Mercury
BEPICOLOMBO - A MISSION TO MERCURY ∗ R. Jehn , J. Schoenmaekers, D. Garc´ıa and P. Ferri European Space Operations Centre, ESA/ESOC, Darmstadt, Germany ABSTRACT BepiColombo is a cornerstone mission of the ESA Science Programme, to be launched towards Mercury in July 2014. After a journey of nearly 6 years two probes, the Magneto- spheric Orbiter (JAXA) and the Planetary Orbiter (ESA) will be separated and injected into their target orbits. The interplanetary trajectory includes flybys at the Earth, Venus (twice) and Mercury (four times), as well as several thrust arcs provided by the solar electric propulsion module. At the end of the transfer a gravitational capture at the weak stability boundary is performed exploiting the Sun gravity. In case of a failure of the orbit insertion burn, the spacecraft will stay for a few revolutions in the weakly captured orbit. The arrival conditions are chosen such that backup orbit insertion manoeuvres can be performed one, four or five orbits later with trajectory correction manoeuvres of less than 15 m/s to compensate the Sun perturbations. Only in case that no manoeuvre can be performed within 64 days (5 orbits) after the nominal orbit insertion the spacecraft will leave Mercury and the mission will be lost. The baseline trajectory has been designed taking into account all operational constraints: 90-day commissioning phase without any thrust; 30-day coast arcs before each flyby (to allow for precise navigation); 7-day coast arcs after each flyby; 60-day coast arc before orbit insertion; Solar aspect angle constraints and minimum flyby altitudes (300 km at Earth and Venus, 200 km at Mercury). -
The Search for Another Earth – Part II
GENERAL ARTICLE The Search for Another Earth – Part II Sujan Sengupta In the first part, we discussed the various methods for the detection of planets outside the solar system known as the exoplanets. In this part, we will describe various kinds of exoplanets. The habitable planets discovered so far and the present status of our search for a habitable planet similar to the Earth will also be discussed. Sujan Sengupta is an 1. Introduction astrophysicist at Indian Institute of Astrophysics, Bengaluru. He works on the The first confirmed exoplanet around a solar type of star, 51 Pe- detection, characterisation 1 gasi b was discovered in 1995 using the radial velocity method. and habitability of extra-solar Subsequently, a large number of exoplanets were discovered by planets and extra-solar this method, and a few were discovered using transit and gravi- moons. tational lensing methods. Ground-based telescopes were used for these discoveries and the search region was confined to about 300 light-years from the Earth. On December 27, 2006, the European Space Agency launched 1The movement of the star a space telescope called CoRoT (Convection, Rotation and plan- towards the observer due to etary Transits) and on March 6, 2009, NASA launched another the gravitational effect of the space telescope called Kepler2 to hunt for exoplanets. Conse- planet. See Sujan Sengupta, The Search for Another Earth, quently, the search extended to about 3000 light-years. Both Resonance, Vol.21, No.7, these telescopes used the transit method in order to detect exo- pp.641–652, 2016. planets. Although Kepler’s field of view was only 105 square de- grees along the Cygnus arm of the Milky Way Galaxy, it detected a whooping 2326 exoplanets out of a total 3493 discovered till 2Kepler Telescope has a pri- date. -
CHORUS: Let's Go Meet the Dwarf Planets There Are Five in Our Solar
Meet the Dwarf Planet Lyrics: CHORUS: Let’s go meet the dwarf planets There are five in our solar system Let’s go meet the dwarf planets Now I’ll go ahead and list them I’ll name them again in case you missed one There’s Pluto, Ceres, Eris, Makemake and Haumea They haven’t broken free from all the space debris There’s Pluto, Ceres, Eris, Makemake and Haumea They’re smaller than Earth’s moon and they like to roam free I’m the famous Pluto – as many of you know My orbit’s on a different path in the shape of an oval I used to be planet number 9, But I break the rules; I’m one of a kind I take my time orbiting the sun It’s a long, long trip, but I’m having fun! Five moons keep me company On our epic journey Charon’s the biggest, and then there’s Nix Kerberos, Hydra and the last one’s Styx 248 years we travel out Beyond the other planet’s regular rout We hang out in the Kuiper Belt Where the ice debris will never melt CHORUS My name is Ceres, and I’m closest to the sun They found me in the Asteroid Belt in 1801 I’m the only known dwarf planet between Jupiter and Mars They thought I was an asteroid, but I’m too round and large! I’m Eris the biggest dwarf planet, and the slowest one… It takes me 557 years to travel around the sun I have one moon, Dysnomia, to orbit along with me We go way out past the Kuiper Belt, there’s so much more to see! CHORUS My name is Makemake, and everyone thought I was alone But my tiny moon, MK2, has been with me all along It takes 310 years for us to orbit ‘round the sun But out here in the Kuiper Belt… our adventures just begun Hello my name’s Haumea, I’m not round shaped like my friends I rotate fast, every 4 hours, which stretched out both my ends! Namaka and Hi’iaka are my moons, I have just 2 And we live way out past Neptune in the Kuiper Belt it’s true! CHORUS Now you’ve met the dwarf planets, there are 5 of them it’s true But the Solar System is a great big place, with more exploring left to do Keep watching the skies above us with a telescope you look through Because the next person to discover one… could be me or you… . -
The Midnight Sky: Familiar Notes on the Stars and Planets, Edward Durkin, July 15, 1869 a Good Way to Start – Find North
The expression "dog days" refers to the period from July 3 through Aug. 11 when our brightest night star, SIRIUS (aka the dog star), rises in conjunction* with the sun. Conjunction, in astronomy, is defined as the apparent meeting or passing of two celestial bodies. TAAS Fabulous Fifty A program for those new to astronomy Friday Evening, July 20, 2018, 8:00 pm All TAAS and other new and not so new astronomers are welcome. What is the TAAS Fabulous 50 Program? It is a set of 4 meetings spread across a calendar year in which a beginner to astronomy learns to locate 50 of the most prominent night sky objects visible to the naked eye. These include stars, constellations, asterisms, and Messier objects. Methodology 1. Meeting dates for each season in year 2018 Winter Jan 19 Spring Apr 20 Summer Jul 20 Fall Oct 19 2. Locate the brightest and easiest to observe stars and associated constellations 3. Add new prominent constellations for each season Tonight’s Schedule 8:00 pm – We meet inside for a slide presentation overview of the Summer sky. 8:40 pm – View night sky outside The Midnight Sky: Familiar Notes on the Stars and Planets, Edward Durkin, July 15, 1869 A Good Way to Start – Find North Polaris North Star Polaris is about the 50th brightest star. It appears isolated making it easy to identify. Circumpolar Stars Polaris Horizon Line Albuquerque -- 35° N Circumpolar Stars Capella the Goat Star AS THE WORLD TURNS The Circle of Perpetual Apparition for Albuquerque Deneb 1 URSA MINOR 2 3 2 URSA MAJOR & Vega BIG DIPPER 1 3 Draco 4 Camelopardalis 6 4 Deneb 5 CASSIOPEIA 5 6 Cepheus Capella the Goat Star 2 3 1 Draco Ursa Minor Ursa Major 6 Camelopardalis 4 Cassiopeia 5 Cepheus Clock and Calendar A single map of the stars can show the places of the stars at different hours and months of the year in consequence of the earth’s two primary movements: Daily Clock The rotation of the earth on it's own axis amounts to 360 degrees in 24 hours, or 15 degrees per hour (360/24). -
Dwarf Planet Ceres
Dwarf Planet Ceres drishtiias.com/printpdf/dwarf-planet-ceres Why in News As per the data collected by NASA’s Dawn spacecraft, dwarf planet Ceres reportedly has salty water underground. Dawn (2007-18) was a mission to the two most massive bodies in the main asteroid belt - Vesta and Ceres. Key Points 1/3 Latest Findings: The scientists have given Ceres the status of an “ocean world” as it has a big reservoir of salty water underneath its frigid surface. This has led to an increased interest of scientists that the dwarf planet was maybe habitable or has the potential to be. Ocean Worlds is a term for ‘Water in the Solar System and Beyond’. The salty water originated in a brine reservoir spread hundreds of miles and about 40 km beneath the surface of the Ceres. Further, there is an evidence that Ceres remains geologically active with cryovolcanism - volcanoes oozing icy material. Instead of molten rock, cryovolcanoes or salty-mud volcanoes release frigid, salty water sometimes mixed with mud. Subsurface Oceans on other Celestial Bodies: Jupiter’s moon Europa, Saturn’s moon Enceladus, Neptune’s moon Triton, and the dwarf planet Pluto. This provides scientists a means to understand the history of the solar system. Ceres: It is the largest object in the asteroid belt between Mars and Jupiter. It was the first member of the asteroid belt to be discovered when Giuseppe Piazzi spotted it in 1801. It is the only dwarf planet located in the inner solar system (includes planets Mercury, Venus, Earth and Mars). Scientists classified it as a dwarf planet in 2006. -
Should Earth Get Demoted from Planet Status Just Like Pluto?
IOSR Journal of Applied Physics (IOSR-JAP) e-ISSN: 2278-4861.Volume 10, Issue 3 Ver. I (May. – June. 2018), PP 15-19 www.iosrjournals.org Should Earth Get Demoted From Planet Status Just Like Pluto? Dipak Nath Assistant Professor, HOD, Department of Physics, Sao Chang Govt College, Tuensang;Nagaland, India. Corresponding Author: Dipak Nath Abstract: Clyde.W. Tombough discovered Pluto on march13, 1930. From its discovery in 1930 until 2006, Pluto was classified as Planet. In the late 20th and early 21st century, many objects similar to Pluto were discovered in the outer solar system, notably the scattered disc object Eris in 2005, which is 27% more massive than Pluto. On august-24, 2006, the International Astronomical Union (IAU) defined what it means to be a Planet within the solar system. This definition excluded Pluto as a Planet added it as a member of the new category “Dwarf Planet” along with Eris and Ceres. There were many reasons why Pluto got demoted to dwarf planet status, one of which was that it couldn't clear its orbit of asteroids and other debris. But Earth's orbit is also crowded...too crowded for Earth to be a planet? Earth is indeed in a very crowded orbit, surrounded by tens of thousands of asteroids and other objects. The presence of so many asteroids seems like a serious problem for Earth's claim that it has cleared its neighborhood. And Earth isn't alone in this problem - Jupiter is surrounded by some 100,000 Trojan asteroids, and there's similar clutter around Mars and Neptune.