SOLAR OBLIQUITY INDUCED by PLANET NINE Elizabeth Bailey, Konstantin Batygin, Michael E
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Current State of Knowledge of the Magnetospheres of Uranus and Neptune
Current State of Knowledge of the Magnetospheres of Uranus and Neptune 28 July 2014 Abigail Rymer [email protected] What does a ‘normal’ magnetosphere look like? . N-S dipole field perpendicular to SW . Solar wind driven circulation system . Well defined central tail plasmasheet . Loaded flux tubes lost via substorm activity . Trapped radiation on closed (dipolar) field lines close to the planet. …but then what is normal…. Mercury Not entirely at the mercy of the solar wind after all . Jupiter . More like its own little solar system . Sub-storm activity maybe totally internally driven …but then what is normal…. Saturn Krimigis et al., 2007 What is an ice giant (as distinct from a gas giant) planet? Consequenses for the magnetic field Soderlund et al., 2012 Consequenses for the magnetic field Herbert et al., 2009 Are Neptune and Uranus the same? URANUS NEPTUNE Equatorial radius 25 559 km 24 622 km Mass 14.5 ME 17.14 ME Sidereal spin period 17h12m36s (retrograde) 16h6m36s Obliquity (axial tilt to ecliptic) -97.77º 28.32 Semi-major axis 19.2 AU 30.1 AU Orbital period 84.3 Earth years 164.8 Earth years Dipole moment 50 ME 25 ME Magnetic field Highly complex with a surface Highly complex with a surface field up to 110 000 nT field up to 60 000 nT Dipole tilt -59º -47 Natural satellites 27 (9 irregular) 14 (inc Triton at 14.4 RN) Spacecraft at Uranus and Neptune – Voyager 2 Voyager 2 observations - Uranus Stone et al., 1986 Voyager 2 observations - Uranus Voyager 2 made excellent plasma measurements with PLS, a Faraday cup type instrument. -
Solar Illumination Conditions at 4 Vesta: Predictions Using the Digital Elevation Model Derived from Hst Images
42nd Lunar and Planetary Science Conference (2011) 2506.pdf SOLAR ILLUMINATION CONDITIONS AT 4 VESTA: PREDICTIONS USING THE DIGITAL ELEVATION MODEL DERIVED FROM HST IMAGES. T. J. Stubbs 1,2,3 and Y. Wang 1,2,3 , 1Goddard Earth Science and Technology Center, University of Maryland, Baltimore County, Baltimore, MD, USA, 2NASA Goddard Space Flight Center, Greenbelt, MD, USA, 3NASA Lunar Science Institute, Ames Research Center, Moffett Field, CA, USA. Corresponding email address: Timothy.J.Stubbs[at]NASA.gov . Introduction: As with other airless bodies in the plane), the longitude of the ascending node is 103.91° Solar System, the surface of 4 Vesta is directly exposed and the argument of perihelion is 149.83°. Based on to the full solar spectrum. The degree of solar illumina- current estimates, Vesta’s orbital plane is believed to tion plays a major role in processes at the surface, in- have a precession period of 81,730 years [6]. cluding heating (surface temperature), space weather- For the shape of Vesta we use the 5 × 5° DEM ing, surface charging, surface chemistry, and exo- based on HST images [5], which is publicly available spheric production via photon-stimulated desorption. from the Planetary Data System (PDS). To our knowl- The characterization of these processes is important for edge, this is the best DEM of Vesta currently available. interepreting various surface properties. It is likely that The orbital information for Vesta is obtained from the solar illumination also controls the transport and depo- Dawn SPICE kernel, which currently limits us to the sition of volatiles at Vesta, as has been proposed at the current epoch (1900 to present). -
Calibration of the Angular Momenta of the Minor Planets in the Solar System Jian Li1, Zhihong Jeff Xia2, Liyong Zhou1
Astronomy & Astrophysics manuscript no. arXiv c ESO 2019 September 26, 2019 Calibration of the angular momenta of the minor planets in the solar system Jian Li1, Zhihong Jeff Xia2, Liyong Zhou1 1School of Astronomy and Space Science & Key Laboratory of Modern Astronomy and Astrophysics in Ministry of Education, Nanjing University, 163 Xianlin Road, Nanjing 210023, PR China e-mail: [email protected] 2Department of Mathematics, Northwestern University, 2033 Sheridan Road, Evanston, IL 60208, USA e-mail: [email protected] September 26, 2019 ABSTRACT Aims. We aim to determine the relative angle between the total angular momentum of the minor planets and that of the Sun-planets system, and to improve the orientation of the invariable plane of the solar system. Methods. By utilizing physical parameters available in public domain archives, we assigned reasonable masses to 718041 minor plan- ets throughout the solar system, including near-Earth objects, main belt asteroids, Jupiter trojans, trans-Neptunian objects, scattered- disk objects, and centaurs. Then we combined the orbital data to calibrate the angular momenta of these small bodies, and evaluated the specific contribution of the massive dwarf planets. The effects of uncertainties on the mass determination and the observational incompleteness were also estimated. Results. We determine the total angular momentum of the known minor planets to be 1:7817 × 1046 g · cm2 · s−1. The relative angle α between this vector and the total angular momentum of the Sun-planets system is calculated to be about 14:74◦. By excluding the dwarf planets Eris, Pluto, and Haumea, which have peculiar angular momentum directions, the angle α drops sharply to 1:76◦; a similar result applies to each individual minor planet group (e.g., trans-Neptunian objects). -
Tilting Saturn II. Numerical Model
Tilting Saturn II. Numerical Model Douglas P. Hamilton Astronomy Department, University of Maryland College Park, MD 20742 [email protected] and William R. Ward Southwest Research Institute Boulder, CO 80303 [email protected] Received ; accepted Submitted to the Astronomical Journal, December 2003 Resubmitted to the Astronomical Journal, June 2004 – 2 – ABSTRACT We argue that the gas giants Jupiter and Saturn were both formed with their rotation axes nearly perpendicular to their orbital planes, and that the large cur- rent tilt of the ringed planet was acquired in a post formation event. We identify the responsible mechanism as trapping into a secular spin-orbit resonance which couples the angular momentum of Saturn’s rotation to that of Neptune’s orbit. Strong support for this model comes from i) a near match between the precession frequencies of Saturn’s pole and the orbital pole of Neptune and ii) the current directions that these poles point in space. We show, with direct numerical inte- grations, that trapping into the spin-orbit resonance and the associated growth in Saturn’s obliquity is not disrupted by other planetary perturbations. Subject headings: planets and satellites: individual (Saturn, Neptune) — Solar System: formation — Solar System: general 1. INTRODUCTION The formation of the Solar System is thought to have begun with a cold interstellar gas cloud that collapsed under its own self-gravity. Angular momentum was preserved during the process so that the young Sun was initially surrounded by the Solar Nebula, a spinning disk of gas and dust. From this disk, planets formed in a sequence of stages whose details are still not fully understood. -
Our Solar System
This graphic of the solar system was made using real images of the planets and comet Hale-Bopp. It is not to scale! To show a scale model of the solar system with the Sun being 1cm would require about 64 meters of paper! Image credit: Maggie Mosetti, NASA This book was produced to commemorate the Year of the Solar System (2011-2013, a martian year), initiated by NASA. See http://solarsystem.nasa.gov/yss. Many images and captions have been adapted from NASA’s “From Earth to the Solar System” (FETTSS) image collection. See http://fettss.arc.nasa.gov/. Additional imagery and captions compiled by Deborah Scherrer, Stanford University, California, USA. Special thanks to the people of Suntrek (www.suntrek.org,) who helped with the final editing and allowed me to use Alphonse Sterling’s awesome photograph of a solar eclipse! Cover Images: Solar System: NASA/JPL; YSS logo: NASA; Sun: Venus Transit from NASA SDO/AIA © 2013-2020 Stanford University; permission given to use for educational and non-commericial purposes. Table of Contents Why Is the Sun Green and Mars Blue? ............................................................................... 4 Our Sun – Source of Life ..................................................................................................... 5 Solar Activity ................................................................................................................... 6 Space Weather ................................................................................................................. 9 Mercury -
Effects of the Moon on the Earth in the Past, Present, and Future
Effects of the Moon on the Earth in the Past, Present, and Future Rina Rast*, Sarah Finney, Lucas Cheng, Joland Schmidt, Kessa Gerein, & Alexandra Miller† Abstract The Moon has fascinated human civilization for millennia. Exploration of the lunar surface played a pioneering role in space exploration, epitomizing the heights to which modern science could bring mankind. In the decades since then, human interest in the Moon has dwindled. Despite this fact, the Moon continues to affect the Earth in ways that seldom receive adequate recognition. This paper examines the ways in which our natural satellite is responsible for the tides, and also produces a stabilizing effect on Earth’s rotational axis. In addition, phenomena such as lunar phases, eclipses and lunar libration will be explained. While investigating the Moon’s effects on the Earth in the past and present, it is hoped that human interest in it will be revitalized as it continues to shape life on our blue planet. Keywords: Moon, Earth, tides, Earth’s axis, lunar phases, eclipses, seasons, lunar libration Introduction lunar phases, eclipses and libration. In recognizing and propagating these effects, the goal of this study is to rekindle the fascination humans once held for the Moon Decades have come and gone since humans’ fascination and space exploration in general. with the Moon galvanized exploration of the galaxy and observation of distant stars. During the Space Race of the 1950s and 1960s, nations strived and succeeded in reaching Four Prominent Lunar Effects on Earth Earth’s natural satellite to propel mankind to new heights. Although this interest has dwindled and humans have Effect on Oceans and Tides largely distanced themselves from the Moon’s relevance, its effects on Earth remain as far-reaching as ever. -
Long Term Behavior of a Hypothetical Planet in a Highly Eccentric Orbit
Long term behavior of a hypothetical planet in a highly eccentric orbit R. Nufer,∗ W. Baltensperger,† W. Woelfli‡ March 29, 2018 Abstract crossed this cloud, molecules activating a Green- house effect were produced in the upper atmosphere For a hypothetical planet on a highly eccentric or- in an amount sufficient to transiently enhance the bit, we have calculated the osculating orbital pa- mean surface temperature on Earth. Very close rameters and its closest approaches to Earth and flyby events even resulted in earthquakes and vol- Moon over a period of 750 kyr. The approaches canic activities. In extreme cases, a rotation of the which are close enough to influence the climate of entire Earth relative to its rotation axis occured in the Earth form a pattern comparable to that of the response to the transient strong gravitational inter- past climatic changes, as recorded in deep sea sedi- action. These polar shifts took place with a fre- ments and polar ice cores. quency of about one in one million years on the average. The first of them was responsible for the major drop in mean temperature, whereas the last 1 Motivation one terminated Earth’s Pleistocene Ice Age 11.5 kyr ago. At present, planet Z does not exist any more. The information on Earth’s past climate obtained The high eccentricity of Z’s orbit corresponds to from deep sea sediments and polar ice cores indi- a small orbital angular momentum. This could be cates that the global temperature oscillated with a transferred to one of the inner planets during a close small amplitude around a constant mean value for encounter, so that Z plunged into the sun. -
Orbital Resonances in the Inner Neptunian System I. the 2:1 Proteus–Larissa Mean-Motion Resonance Ke Zhang ∗, Douglas P
Icarus 188 (2007) 386–399 www.elsevier.com/locate/icarus Orbital resonances in the inner neptunian system I. The 2:1 Proteus–Larissa mean-motion resonance Ke Zhang ∗, Douglas P. Hamilton Department of Astronomy, University of Maryland, College Park, MD 20742, USA Received 1 June 2006; revised 22 November 2006 Available online 20 December 2006 Abstract We investigate the orbital resonant history of Proteus and Larissa, the two largest inner neptunian satellites discovered by Voyager 2.Due to tidal migration, these two satellites probably passed through their 2:1 mean-motion resonance a few hundred million years ago. We explore this resonance passage as a method to excite orbital eccentricities and inclinations, and find interesting constraints on the satellites’ mean density 3 3 (0.05 g/cm < ρ¯ 1.5g/cm ) and their tidal dissipation parameters (Qs > 10). Through numerical study of this mean-motion resonance passage, we identify a new type of three-body resonance between the satellite pair and Triton. These new resonances occur near the traditional two-body resonances between the small satellites and, surprisingly, are much stronger than their two-body counterparts due to Triton’s large mass and orbital inclination. We determine the relevant resonant arguments and derive a mathematical framework for analyzing resonances in this special system. © 2007 Elsevier Inc. All rights reserved. Keywords: Resonances, orbital; Neptune, satellites; Triton; Satellites, dynamics 1. Introduction Most of the debris was probably swept up by Triton (Cuk´ and Gladman, 2005), while some material close to Neptune sur- Prior to the Voyager 2 encounter, large icy Triton and dis- vived to form a new generation of satellites with an accretion tant irregular Nereid were Neptune’s only known satellites. -
Exploring the Orbital Evolution of Planetary Systems
Exploring the orbital evolution of planetary systems Tabar´e Gallardo∗ Instituto de F´ısica, Facultad de Ciencias, Udelar. (Dated: January 22, 2017) The aim of this paper is to encourage the use of orbital integrators in the classroom to discover and understand the long term dynamical evolution of systems of orbiting bodies. We show how to perform numerical simulations and how to handle the output data in order to reveal the dynamical mechanisms that dominate the evolution of arbitrary planetary systems in timescales of millions of years using a simple but efficient numerical integrator. Trough some examples we reveal the fundamental properties of the planetary systems: the time evolution of the orbital elements, the free and forced modes that drive the oscillations in eccentricity and inclination, the fundamental frequencies of the system, the role of the angular momenta, the invariable plane, orbital resonances and the Kozai-Lidov mechanism. To be published in European Journal of Physics. 2 I. INTRODUCTION With few exceptions astronomers cannot make experiments, they are limited to observe the universe. The laboratory for the astronomer usually takes the form of computer simulations. This is the most important instrument for the study of the dynamical behavior of gravitationally interacting bodies. A planetary system, for example, evolves mostly due to gravitation acting over very long timescales generating what is called a secular evolution. This secular evolution can be deduced analytically by means of the theory of perturbations, but can also be explored in the classroom by means of precise numerical integrators. Some facilities exist to visualize and experiment with the gravitational interactions between massive bodies1–3. -
Forced Obliquities and Moments of Inertia of Ceres and Vesta ⇑ B.G
Icarus 213 (2011) 496–509 Contents lists available at ScienceDirect Icarus journal homepage: www.elsevier.com/locate/icarus Forced obliquities and moments of inertia of Ceres and Vesta ⇑ B.G. Bills a, , F. Nimmo b a Jet Propulsion Laboratory, Pasadena, CA 91109, USA b Department of Earth and Planetary Sciences, University of California Santa Cruz, Santa Cruz, CA 95064, USA article info abstract Article history: We examine models of secular variations in the orbit and spin poles of Ceres and Vesta, the two most Received 22 July 2009 massive bodies in the main asteroid belt. If the spin poles are fully damped, then the current values of Revised 30 August 2010 obliquity, or angular separation between spin and orbit poles, are diagnostic of the moments of inertia Accepted 1 September 2010 and thus indicative of the extent of differentiation of these bodies. Using existing shape models and Available online 21 September 2010 assuming uniform density, the present obliquity values are predicted to be 12.31° for Ceres and 15.66° for Vesta. Part of this difference is related to differing orbital inclinations; a more centrally condensed Keywords: internal structure would yield more rapid spin pole precession, and larger obliquity. Time scales for tidal Asteroids, Dynamics damping are expected to be rather long. However, at least for Vesta, current estimates of the spin pole Asteroid Ceres Asteroid Vesta location are consistent with its obliquity being fully damped. When the degree two gravity coefficients Rotational dynamics and spin pole orientations are determined by the Dawn spacecraft, it will allow accurate determination of the moments of inertia of these bodies, assuming the obliquities are damped. -
Astro 250: Solutions to Problem Set 5 by Eugene Chiang
Astro 250: Solutions to Problem Set 5 by Eugene Chiang Problem 1. Precessing Planes and the Invariable Plane Consider a star of mass mc orbited by two planets on nearly circular orbits. The mass and semi-major axis of the inner planet are m1 and a1, respectively, and those of the outer planet, m2 = (1/2) × m1 and a2 = 4 × a1. The mutual inclination between the two orbits is i 1. This problem explores the inclination and nodal behavior of the two planets. a) What is the inclination of each planet with respect to the invariable plane of the system? The invariable plane is perpendicular to the total (vector) angular momentum of all planetary orbits. Neglect the contribution of orbital eccentricity to the angular momentum. Call these inclinations i1 and i2. The masses and semi-major axes of the two planets are so chosen as to make the arithmetic easy;√ the norm of each planet’s angular momentum is the same as the other, |~l1| = |~l2| = m1 Gmca1. Orient the x-y axes in the invariable plane so that the y-axis lies along the line of intersection between the two orbit planes (the nodal line). Then in the x-z plane, the total angular momentum vector lies along the z-axis, while ~l1 lies (say) in quadrant II and makes an angle with respect to the z-axis of i1 > 0, while l~2 lies in quadrant I and makes an angle with respect to the z-axis of i2 > 0. Remember that the mutual inclination i = i1 + i2. -
On the Irrelevance of Being a PLUTO! Size Scale of Stars and Planets
On the irrelevance of being a PLUTO! Mayank Vahia DAA, TIFR Irrelevance of being Pluto 1 Size Scale of Stars and Planets Irrelevance of being Pluto 2 1 1 AU 700 Dsun Irrelevance of being Pluto 3 16 Dsun Irrelevance of being Pluto 4 2 Solar System 109 DEarth Irrelevance of being Pluto 5 11 DEarth Venus Irrelevance of being Pluto 6 3 Irrelevance of being Pluto 7 Solar System visible to unaided eye Irrelevance of being Pluto 8 4 Solar System at the beginning of 20 th Century Irrelevance of being Pluto 9 Solar System of my text book (30 years ago) Irrelevance of being Pluto 10 5 Asteroid Belt (Discovered in 1977) Irrelevance of being Pluto 11 The ‘Planet’ Pluto • Pluto is a 14 th magnitude object. • It is NOT visible to naked eye (neither are Uranus and Neptune). • It was discovered by American astronomer Clyde Tombaugh in 1930. Irrelevance of being Pluto 12 6 Prediction of Pluto • Percival Lowell and William H. Pickering are credited with the theoretical work on Pluto’s orbit done in 1909 based on data of Neptune’s orbital changes. • Venkatesh Ketakar had predicted it in May 1911 issue of Bulletin of the Astronomical Society of France. • He modelled his computations after those of Pierre-Simon Laplace who had analysed the motions of the satellites of Jupiter. • His location was within 1 o of its correct location. • He had predicted ts orbital period was 242.28 (248) years and a distance of 38.95 (39.53) A.U. • He had also predicted another planet at 59.573 A.U.