Twenty Reasons Why Pluto Should Still Be a Planet
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11000 Scientists Around the World Have the Final Say on What's a Planet
International Astronomical Union (IAU) members vote on a new planet definition during a meeting in Prague Aug. 24, 2006. The vote redefined Pluto as a dwarf planet. MICHAL CIZEK/AFP/GETTY IMAGES DEFINITION: PLANET 11,000 scientists around the world have the final say on what’s a planet — or not By Mary Helen Berg a planet is a planet or just an orbiting ice of planetary scientists, academics and ball. Right now, the worlds that make historians support research, confirm HE NUMBER OF PLANETS IN OUR the cut are Mercury, Venus, Earth, Mars, celestial discoveries, document and solar system is … well, it depends Jupiter, Saturn, Uranus and Neptune. preserve data and even track potentially on who you ask. Pluto fans, sporting The IAU is “responsible for managing the dangerous asteroids. T-shirts that read “Never Forget,” astronomical world,” said Gareth Williams, Tstill say there are nine. Meanwhile, some associate director of the NASA-funded IAU PLUTO OUT astronomers say the tally should be 13. But Minor Planet Center (MPC). “They define Most of these working groups fly under the arbiter on all things astronomical, the everything that astronomers need to talk the radar. But in 2006, one committee International Astronomical Union (IAU), about objects in a consistent way. So, if I’m found itself under global scrutiny when, for recognizes only eight planets. talking about an object at a certain point the first time, the astronomy community As the world’s largest professional in the sky, some other astronomer knows demanded an official definition of “planet.” organization for astronomers, the IAU exactly what I am talking about.” The seven-member Planet Definition represents 11,000 scientists from 95 In other words, the IAU controls cosmic countries and has the final say on whether chaos on Earth. -
What Is a Planet? Published on Division for Planetary Sciences (
What is a Planet? Published on Division for Planetary Sciences (https://dps.aas.org) What is a Planet? 11 October 2006 On Wednesday, August 16, 2006, the International Astronomical Union (IAU) announced a proposed definition of a planet. A significantly revised version of this definition was passed by the membership at its general meeting on August 24, 2006. The IAU is an international organization of over 8,000 astronomers representing over 80 countries and held its meeting this year in Prague. The proposal for defining “what is a planet” and the fate of Pluto has been making front-page news for several weeks. In the draft resolution, three “planets” (asteroid Ceres, distant object 2003 UB313, and Pluto's satellite Charon) were added to the existing nine planets. However, there was concern by many astronomers that, if this definition of a planet passed, there was the likelihood that dozens of other planets would be added in the near future. A summary [1] of what went on in Prague, the process that led to the final vote on August 24, the concerns that have since been raised by some astronomers, and the process that will lead to an eventual formulation for the definition of a planet was sent by Dr. Richard French, DPS Chair, to the entire DPS membership. What brought about this proposal? In 1930, when Pluto was discovered by Clyde Tombaugh, it was thought to be as large as Earth. With more study, we now know that it is only a little more than 2200 km in diameter, smaller than our Moon! For this reason, during the 1990s, a few astronomers began questioning whether or not Pluto should be considered a planet. -
What Is a Planet?
What is a Planet? Steven Soter Department of Astrophysics, American Museum of Natural History, Central Park West at 79th Street, New York, NY 10024, and Center for Ancient Studies, New York University [email protected] submitted to The Astronomical Journal 16 Aug 2006, published in Vol. 132, pp. 2513-2519 Abstract. A planet is an end product of disk accretion around a primary star or substar. I quantify this definition by the degree to which a body dominates the other masses that share its orbital zone. Theoretical and observational measures of dynamical dominance reveal gaps of four to five orders of magnitude separating the eight planets of our solar system from the populations of asteroids and comets. The proposed definition dispenses with upper and lower mass limits for a planet. It reflects the tendency of disk evolution in a mature system to produce a small number of relatively large bodies (planets) in non-intersecting or resonant orbits, which prevent collisions between them. 1. Introduction Beginning in the 1990s astronomers discovered the Kuiper Belt, extrasolar planets, brown dwarfs, and free-floating planets. These discoveries have led to a re-examination of the conventional definition of a “planet” as a non-luminous body that orbits a star and is larger than an asteroid (see Stern & Levison 2002, Mohanty & Jayawardhana 2006, Basri & Brown 2006). When Tombaugh discovered Pluto in 1930, astronomers welcomed it as the long sought “Planet X”, which would account for residual perturbations in the orbit of Neptune. In fact those perturbations proved to be illusory, and the discovery of Pluto was fortuitous. -
Geophysical Classification of Planets, Dwarf Planets, and Moons: a Mass Scale and Composition Codes David G
- 1 - Geophysical Classification of Planets, Dwarf Planets, and Moons: A Mass Scale and Composition Codes David G. Russell Owego Free Academy, Owego, NY USA [email protected] [email protected] Abstract A planetary mass scale and system of composition codes are presented for describing the geophysical characteristics of exoplanets and Solar System planets, dwarf planets, and spherical moons. The composition classes characterize the rock, ice, and gas properties of planetary bodies. The planetary mass scale includes five mass classes with upper and lower mass limits derived from recent studies of the exoplanet mass-radius and mass-density relationships, and the physical characteristics of planets, dwarf planets, and spherical moons in the Solar System. The combined mass and composition codes provide a geophysical classification that allows for comparison of the global mass and composition characteristics of exoplanets with the Solar System’s planets, dwarf planets and spherical moons. The system is flexible and can be combined with additional codes characterizing other physical, dynamical, or biological characteristics of planets. Subject Headings: planets and satellites: composition - planets and satellites: fundamental parameters - planets and satellites: general 1. Introduction To date nearly 3000 exoplanets have been confirmed (Han et al. 2014). It is possible to derive reasonable models for the interior structure of most Solar System planets and many exoplanets (Baraffe et al. 2008, 2010, 2014; Fortney et al. 2006, Sotin et al. 2010). Numerous names are used to characterize exoplanets including: Earth, super-Earth, mini-Neptune, Neptune, sub-Neptune, hot Neptune, Saturn, Jupiter, hot Jupiter, Jovian, gas giant, ice giant, rocky, terrestrial, water, and ocean. -
A Geophysical Planet Definition
Lunar and Planetary Science XLVIII (2017) 1448.pdf A GEOPHYSICAL PLANET DEFINITION. K.D. Runyon1, S.A. Stern2, T.R. Lauer3, W. Grundy4, M.E. Sum- mers5, K.N. Singer2, 1Johns Hopkins University, Dept. of Earth and Planetary Sciences, Baltimore, MD, USA (kir- [email protected]), 2Southwest Research Institute, Boulder, CO, USA, 3National Optical Astronomy Observa- tory, Tucson, AZ, USA, 4Lowell Observatory, Flagstaff, AZ, USA 5George Mason University, Dept. of Physics and Astronomy, Fairfax, VA, USA. Introduction: In the mind of the public, the word for the given name of the world, even if the world is a “planet” carries a significance lacking in other words moon or dwarf planet. An instance of this usage of used to describe planetary bodies. In the decade fol- “planet” when referring to the moon-planet Titan is, lowing the supposed “demotion” of Pluto by the Inter- “A planet-wide detached haze layer occurs between national Astronomical Union (IAU) [1], many mem- 300-350 km above the surface; the visible limb of the bers of the public, in our experience, assume that al- planet, where the vertical haze optical depth is 0.1, is leged “non-planets” cease to be interesting enough to about 220 km above the surface” [4]. Another instance warrant scientific exploration, though the IAU did not in the literature refers to Eris, Makemake, and Haumea intend this consequence [1]. To wit: a common ques- as “small planets of the Kuiper Belt” [5]. tion we receive is, “Why did you send New Horizons The IAU Definition: The planet definition adopted to Pluto if it’s not a planet anymore?” To mitigate this by the IAU in 2006 [1] is technically flawed, for sever- unfortunate perception, we propose a new definition of al reasons. -
ASTR-101 Section 004 Lecture 7 Comparative Planetology: The
ASTR-101 Section 004 Lecture 8 Introduction to the Solar System John T. McGraw, Professor Danielle - Theater Operations Test 1 Results • Max Score 76 out of 85. • Curve set at 78: 3 A’s 7 B’s 8 C’s 4 D’s 1 F’ • Did I score your test correctly? • Do you think a question it is unfair or has the wrong answer? 64% Earthlike and Jupiter-like The Terrestrial and Jovian Planets • The four inner planets are called terrestrial planets • Relatively small (with diameters of 5000 to 13,000 km) • High average densities (4000 to 5500 kg/m3) • Composed primarily of rocky materials • The four giant outer planets are called Jovian planets • Large diameters (50,000 to 143,000 km) • Low average densities (700 to 1700 kg/m3) • Composed primarily of hydrogen and helium gas. Pluto •Pluto is a special case • Smaller than any of the terrestrial planets • Intermediate average density of about 1900 kg/m3 • Density suggests it is composed of a mixture of ice and rock • Many Pluto-like Kuiper Belt Objects (KBOs) are now known • Pluto was discovered by Clyde Tombaugh, long-time professor at NMSU. By NM State Law, Pluto remains a “planet!” Definition of a planet • The definition of planet set in August 2006 by the International Astronomical Union (IAU) states that, in the Solar System, a planet is a celestial body which: 1. is in orbit around the Sun, 2. has sufficient mass to assume hydrostatic equilibrium (a nearly round shape), and 3. has "cleared the neighborhood" around its orbit. Dwarf Planets • A dwarf planet is a planetary-mass object that is neither a planet nor a natural satellite. -
“From Planetesimals to Brown Dwarfs: What Is a Planet
Planetesimals to Brown Dwarfs: What is a Planet? Gibor Basri Astronomy Dept. MC3411, Univ. of California, Berkeley, CA 94720-3411 Michael E. Brown Div. of Geological and Planetary Science, Calif. Inst. Of Technology M/C 150-21, Pasadena, CA 91125 Key Words planets, extra-solar planets, Kuiper Belt, planetesimals, brown dwarfs • Abstract The past 15 years have brought about a revolution in our understanding of our Solar System and other planetary systems. During this time, discoveries include the first Kuiper Belt Objects, the first brown dwarfs, and the first extra-solar planets. Although discoveries continue apace, they have called into question our previous perspectives on planets, both here and elsewhere. The result has been a debate about the meaning of the word “planet” itself. It became clear that scientists do not have a widely accepted or clear definition of what a planet is, and both scientists and the public are confused (and sometimes annoyed) by its use in various contexts. Because “planet” is a very widely used term, it seems worth the attempt to resolve this problem. In this essay, we try to cover all the issues that have come to the fore, and bring clarity (if not resolution) to the debate. Introduction Since prehistoric times, people looked into the night sky and picked out the planets. It was easy: they were the stars that moved (initially the Greeks considered the Sun and Moon to be planets too). Even when Galileo found that the planets are other worlds (and that the Earth is one too), there was no real controversy about what planets were. -
Book of Abstracts 2009 European Week of Astronomy and Space
rs uvvwxyuzyws { yz|z|} rsz}~suzywsu}u~w vz~wsw 456789@A C 99D 7EFGH67A7I P @AQ R8@S9 RST9AS9 UVWUX `abcdUVVe fATg96GTHP7Eh96HE76QGiT69pf q rAS76876@HTAs tFR u Fv wxxy @AQ 4FR 4u Fv wxxy UVVe abbc d dbdc e f gc hi` ij ad bch dgcadabdddc c d ac k lgbc bcgb dmg agd g` kg bdcd dW dd k bg c ngddbaadgc gabmob nb boglWad g kdcoddog kedgcW pd gc bcogbpd kb obpcggc dd kfq` UVVe c iba ! " #$%& $' ())01023 Book of Abstracts – Table of Contents Welcome to the European Week of Astronomy & Space Science ...................................................... iii How space, and a few stars, came to Hatfield ............................................................................... v Plenary I: UK Solar Physics (UKSP) and Magnetosphere, Ionosphere and Solar Terrestrial (MIST) ....... 1 Plenary II: European Organisation for Astronomical Research in the Southern Hemisphere (ESO) ....... 2 Plenary III: European Space Agency (ESA) .................................................................................. 3 Plenary IV: Square Kilometre Array (SKA), High-Energy Astrophysics, Asteroseismology ................... 4 Symposia (1) The next era in radio astronomy: the pathway to SKA .............................................................. 5 (2) The standard cosmological models - successes and challenges .................................................. 17 (3) Understanding substellar populations and atmospheres: from brown dwarfs to exo-planets .......... 28 (4) The life cycle of dust ........................................................................................................... -
Unit 7: Comparing Planets
Unit 7: Comparing Planets This material was developed by the Friends of the Dominion Astrophysical Observatory with the assistance of a Natural Science and Engineering Research Council PromoScience grant and the NRC. It is a part of a larger project to present grade-appropriate material that matches 2020 curriculum requirements to help students understand planets, with a focus on exoplanets. This material is aimed at BC Grade 6 students. French versions are available. Instructions for teachers ● For questions and to give feedback contact: Calvin Schmidt [email protected], ● All units build towards the Big Idea in the curriculum showing our solar system in the context of the Milky Way and the Universe, and provide background for understanding exoplanets. ● Look for Ideas for extending this section, Resources, and Review and discussion questions at the end of each topic in this Unit. These should give more background on each subject and spark further classroom ideas. We would be happy to help you expand on each topic and develop your own ideas for your students. Contact us at the [email protected]. Instructions for students ● If there are parts of this unit that you find confusing, please contact us at [email protected] for help. ● We recommend you do a few sections at a time. We have provided links to learn more about each topic. ● You don’t have to do the sections in order, but we recommend that. Do sections you find interesting first and come back and do more at another time. ● It is helpful to try the activities rather than just read them. -
International Astronomical Union Union Astronomique Internationale
INTERNATIONAL ASTRONOMICAL UNION UNION ASTRONOMIQUE INTERNATIONALE ************ IAU0603: FOR IMMEDIATE RELEASE ************ http://www.iau2006.org/mirror/www.iau.org/iau0603/index.html IAU 2006 General Assembly: Result of the IAU Resolution votes 24-August-2006, Prague: The first half of the Closing Ceremony of the 2006 International Astronomical Union (IAU) General Assembly has just concluded. The results of the Resolution votes are outlined here. It is official: The 26th General Assembly for the International Astronomical Union was an astounding success! More than 2500 astronomers participated in six Symposia, 17 Joint Discussions, seven Special Sessions and four Special Sessions. New science results were vigorously discussed, new international collaborations were initiated, plans for future facilities put forward and much more. In addition to all the exciting astronomy discussed at the General Assembly, six IAU Resolutions were also passed at the Closing Ceremony of the General Assembly: 1. Resolution 1 for GA-XXVI : “Precession Theory and Definition of the Ecliptic” 2. Resolution 2 for GA-XXVI: “Supplement to the IAU 2000 Resolutions on reference systems” 3. Resolution 3 for GA-XXVI: “Re-definition of Barycentric Dynamical Time, TDB” 4. Resolution 4 for GA-XXVI: “Endorsement of the Washington Charter for Communicating Astronomy with the Public” 5. Resolution 5A: “Definition of ‘planet’ ” 6. Resolution 6A: “Definition of Pluto-class objects” The IAU members gathered at the 2006 General Assembly agreed that a “planet” is defined as a celestial body that (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 neighbourhood around its orbit. -
Planets in Our Solar System Compiled by Terra Nova Reading Practice Sets Terranovamd.Com
PLANETS IN OUR SOLAR SYSTEM READING PRACTICE SETS COMPILED FOR YOU BY TERRA NOVA ENGLISH LANGUAGE CENTER LANGUAGE ENGLISH NOVA BY TERRA YOU FOR COMPILED TOEFL iBT READING PRACTICE SET PLANETS IN OUR SOLAR SYSTEM COMPILED BY TERRA NOVA READING PRACTICE SETS TERRANOVAMD.COM Directions: Read the passage and answer the questions. Give yourself 18 minutes to complete this practice set. PLANETS IN OUR SOLAR SYSTEM ❶ The Sun is the hub of a huge rotating system consisting of eight planets and their satellites, dwarf planets, and numerous small bodies, including asteroids, comets, and meteoroids. An estimated 99.86 percent of the mass of our solar system is contained within the Sun, while the planets collectively make up almost all of the remaining 0.14 percent. The planets, in order of their distance from the Sun, are Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, and Neptune. Under the control of the Sun’s gravitational force, each planet maintains an elliptical orbit and all of them travel in the same direction. ❷ The planets in our solar system fall into two groups: the terrestrial (Earth-like) planets (Mercury, Venus, Earth, and Mars) and the Jovian (Jupiter-like) planets (Jupiter, Saturn, Uranus, and Neptune). When Pluto was discovered by Clyde Tombaugh in 1930, it was considered to be the ninth planet. This changed in 2006, when the International Astronomical Union (IAU) adopted a formal definition of “planet,” which reclassified Pluto as a dwarf planet. ❸ The most obvious difference between the terrestrial and the Jovian planets is their size. The largest terrestrial planet, Earth, has a diameter only one quarter as great as the diameter of the smallest Jovian planet, Neptune, and its mass is only one seventeenth as great. -
DPS 50 12OCT2018.Pdf
Program Schedule and Abstract Book DPS 50 October 19 - 27, 2018 The Program Report was last updated October 12, 2018 at 01:30 AM EDT. To view the most recent meeting schedule online, visit https://dps50.abstractcentral.com/planner.jsp Friday, October 19, 2018 You have nothing scheduled for this day Saturday, October 20, 2018 You have nothing scheduled for this day Sunday, October 21, 2018 Time Session or Event Info 8:30 AM-4:30 PM, 200 D (Knoxville Convention Center), DPS Committee Meeting, Attendee Event 10:00 AM-10:30 AM, 301 D (Knoxville Convention Center), DPS Volunteer Orientation, Attendee Event 1:00 PM-5:00 PM, 301 D (Knoxville Convention Center), Bystander Intervention Training, Workshop, Organizer: Sarah Horst, [email protected], John Hopkins University 1:00 PM-6:00 PM, 301 B (Knoxville Convention Center), Juno and Juno-supporting Jupiter Atmospheric Results , Workshop, Organizer: Glenn Orton, [email protected], Jet Propulsion Laboratory, California Institute of Technology 1:00 PM-8:00 PM, Henley Concourse (Knoxville Convention Center), DPS Registration and Badge Pickup, Attendee Event 3:00 PM-4:30 PM, 301 C (Knoxville Convention Center), DPS Early Career Presenters Review, Workshop 3:00 PM-6:00 PM, Ballroom F-G (Knoxville Convention Center), Primitive or Processed? Carbon in Today’s Solar System vs. the early Solar System and the Interstellar Medium, Workshop 3:30 PM-6:30 PM, 301 A (Knoxville Convention Center), Speaker Ready Room, Attendee Event 5:00 PM-6:30 PM, 200 A-C (Knoxville Convention Center), AAS DPS Student