Jupitor's Great Red Spot
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The Acceler the Accelerating Circulation of Jupiter's Great Red
The accelerating circulation of Jupiter’s Great Red Spot John H. Rogers A report of the Jupiter Section (Director: John H. Rogers) Jupiter’s Great Red Spot (GRS) has been evolving, with fluctuations, since it was first observed in the 19th century. It has shown trends of decreasing length, decelerating drift rate, and possibly accelerating internal circulation. This paper documents how these trends have pro- gressed since the time of the Voyager encounters in 1979, up to 2006, from ground-based amateur observations.1 The trends in length and drift rate have continued; the GRS is now smaller than ever before.2 The internal circulation period was directly measured in 2006 for the first time since the Voyager flybys, and is now 4.5 days, which confirms that the period is shortening.3 In contrast, the 90-day oscillation of the GRS in longitude continues unchanged, and may be accompanied by a very small oscillation in latitude. Introduction =–110, +105°/month: the mean speed of the SEBs and STBn jets) through 63 m/s (DL2 = +130°/month: the mean speed of the SEBs jet when a STropD is present) to 110–140 m/s (the The Great Red Spot (GRS) is a giant anticyclone in Jupiter’s maximum internal wind speed recorded in the Voyager im- atmosphere, circulating anticlockwise, with winds that are ages: Table 1a). Images by the Galileo Orbiter in 2000 re- among the most rapid in the solar system (see reference 1, corded a further acceleration to ~145–190 m/s.11,12 pp.188-197). The circulation was already suspected in the These wind speeds were derived by tracking small cloud early 20th century (ref.1, p.256), and the first tentative obser- tracers over short intervals in spacecraft images. -
Planets of the Solar System
Chapter Planets of the 27 Solar System Chapter OutlineOutline 1 ● Formation of the Solar System The Nebular Hypothesis Formation of the Planets Formation of Solid Earth Formation of Earth’s Atmosphere Formation of Earth’s Oceans 2 ● Models of the Solar System Early Models Kepler’s Laws Newton’s Explanation of Kepler’s Laws 3 ● The Inner Planets Mercury Venus Earth Mars 4 ● The Outer Planets Gas Giants Jupiter Saturn Uranus Neptune Objects Beyond Neptune Why It Matters Exoplanets UnderstandingU d t di theth formationf ti and the characteristics of our solar system and its planets can help scientists plan missions to study planets and solar systems around other stars in the universe. 746 Chapter 27 hhq10sena_psscho.inddq10sena_psscho.indd 774646 PDF 88/15/08/15/08 88:43:46:43:46 AAMM Inquiry Lab Planetary Distances 20 min Turn to Appendix E and find the table entitled Question to Get You Started “Solar System Data.” Use the data from the How would the distance of a planet from the sun “semimajor axis” row of planetary distances to affect the time it takes for the planet to complete devise an appropriate scale to model the distances one orbit? between planets. Then find an indoor or outdoor space that will accommodate the farthest distance. Mark some index cards with the name of each planet, use a measuring tape to measure the distances according to your scale, and place each index card at its correct location. 747 hhq10sena_psscho.inddq10sena_psscho.indd 774747 22/26/09/26/09 111:42:301:42:30 AAMM These reading tools will help you learn the material in this chapter. -
Jupiter's “Red Spot Jr.”
National Aeronautics and Space Administration Jupiter’s “Red Spot Jr.” Astronomers Watch the Birth of a Monster Storm Monstrous hurricanes on Earth can stretch across in the close-up image are clouds being shaped by the entire eastern United States. These storms, how- high-speed winds. ever, would be considered timid on Jupiter, where an On Earth, meteorologists routinely watch hur- oval-shaped spot about the size of Earth has recently ricanes form off the African coast, sweep across the emerged. Dubbed Red Spot Jr., this gigantic storm is Atlantic Ocean, and fall apart when they reach the only the little brother of Jupiter’s trademark Great Red colder waters of the northern Atlantic. Astronomers, Spot. however, rarely get the chance to witness the birth of The Great Red Spot is a mammoth oval disturbance storms on our solar system neighbors. Other planets that is so large it could swallow nearly three Earths. are far away from Earth, so astronomers need power- First spotted in 1664 by Robert Hooke, the storm has ful telescopes like the Hubble Space Telescope to been raging on the planet for at least 342 years. track planetary weather. Storms on other planets also Red Spot Jr. is the first storm that astronomers may take years to form. watched develop on a gas giant planet. The huge spot Amateur and professional astronomers eagerly formed between 1998 and 2000, when three small, watched the emerging new red spot. Months later, white, oval-shaped storms merged together. Two of Hubble snapped the first detailed images of Red Spot the white spots have been observed since about 1915, Jr. -
Shades of Blue
Episode # 101 Script # 101 SHADES OF BLUE “Pilot” Written by Adi Hasak Directed by Barry Levinson First Network Draft January 20th, 2015 © 20____ Universal Television LLC ALL RIGHTS RESERVED. NOT TO BE DUPLICATED WITHOUT PERMISSION. This material is the property of Universal Television LLC and is intended solely for use by its personnel. The sale, copying, reproduction or exploitation of this material, in any form is prohibited. Distribution or disclosure of this material to unauthorized persons is also prohibited. PRG-17UT 1 of 1 1-14-15 TEASER FADE IN: INT. MORTUARY PREP ROOM - DAY CLOSE ON the Latino face of RAUL (44), both mortician and local gang leader, as he speaks to someone offscreen: RAUL Our choices define us. It's that simple. A hint of a tattoo pokes out from Raul's collar. His latex- gloved hand holding a needle cycles through frame. RAUL Her parents chose to name her Lucia, the light. At seven, Lucia used to climb out on her fire escape to look at the stars. By ten, Lucia could name every constellation in the Northern Hemisphere. (then) Yesterday, Lucia chose to shoot heroin. And here she lies today. Reveal that Raul is suturing the mouth of a dead YOUNG WOMAN lying supine on a funeral home prep table. As he works - RAUL Not surprising to find such a senseless loss at my doorstep. What is surprising is that Lucia picked up the hot dose from a freelancer in an area I vacated so you could protect parks and schools from the drug trade. I trusted your assurance that no one else would push into that territory. -
Thermal Structure and Composition of Jupiter's Great Red Spot from High-Resolution Thermal Imaging
Thermal Structure and Composition of Jupiter’s Great Red Spot from High-Resolution Thermal Imaging Leigh N. Fletchera,b, G. S. Ortona, O. Mousisc,d, P. Yanamandra-Fishera, P. D. Parrishe,a, P. G. J. Irwinb, B. M. Fishera, L. Vanzif, T. Fujiyoshig, T. Fuseg, A.A. Simon-Millerh, E. Edkinsi, T.L. Haywardj, J. De Buizerk aJet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, CA, 91109, USA bAtmospheric, Oceanic and Planetary Physics, Department of Physics, University of Oxford, Clarendon Laboratory, Parks Road, Oxford, OX1 3PU, UK cInstitut UTINAM, CNRS-UMR 6213, Observatoire de Besan¸con, Universit´ede Franche-Comt´e, Besan¸con, France dLunar and Planetary Laboratory, University of Arizona, Tucson, AZ, USA eSchool of GeoScience, University of Edinburgh, Crew Building, King’s Buildings, Edinburgh, EH9 3JN, UK fPontificia Universidad Catolica de Chile, Department of Electrical Engineering, Av. Vicuna Makenna 4860, Santiago, Chile. gSubaru Telescope, National Astronomical Observatory of Japan, National Institutes of Natural Sciences, 650 North A’ohoku Place, Hilo, Hawaii 96720, USA hNASA/Goddard Spaceflight Center, Greenbelt, Maryland, 20771, USA iUniversity of California, Santa Barbara, Santa Barbara, CA 93106, USA jGemini Observatory, Southern Operations Center, c/o AURA, Casilla 603, La Serena, Chile. kSOFIA - USRA, NASA Ames Research Center, Moffet Field, CA 94035, USA. Abstract Thermal-IR imaging from space-borne and ground-based observatories was used to investigate the temperature, composition and aerosol structure of Jupiter’s Great Red Spot (GRS) and its temporal variability between 1995-2008. An elliptical warm core, extending over 8◦ of longitude and 3◦ of latitude, was observed within the cold anticyclonic vortex at 21◦S. -
The Turbulent Wake of the Jupiter's Great Red Spot Observed with MAD
The Turbulent Wake of the Jupiter's Great Red Spot observed with MAD F. Marchis (UC-Berkeley), M. Wong (UC-Berkeley), E. Marchetti (ESO), J. Kolb (ESO) ABSTRACT The turbulent wake of Jupiter's Great Red Spot (GRS) is a dynamic region known for its massive convective supercells, strong horizontal humidity contrasts, widespread vertical motions, and active heat transport. Attention has recently been drawn to a similar large disorganized feature at the same latitude--but on the other side of the planet. This feature, called a South Equatorial Belt (SEB) outbreak by amateur astronomers, seems to exist independent of the GRS and calls into question the assumed causal relationship between the GRS and its turbulent wake. We propose high-resolution imaging of Jupiter to measure velocities in the SEB outbreak, placing constraints on its dynamic properties. A configuration in August 19 (UT) with two Galilean satellites located on each side of Jupiter was found to be the more appropriate for this observation. This is a time critical observation. SCIENTIFIC CASE High spatial resolution is required to derive velocity fields of Jupiter's atmosphere. Velocity fields of sufficient quality have been obtained from data acquired by orbiter and flyby missions (Voyager, Galileo, Cassini, New Horizons) as well as by the Hubble Space Telescope's ACS (e.g., Mitchell et al. 1981, Simon-Miller et al. 2002, 2006, Choi et al. 2007, Asay-Davis et al. 2008). Data from HST's WFPC2 have resulted in velocity fields of poorer quality, due partly to the unfavorable noise characteristics of the instrument and partly to the sub-sampled point-spread function (pixel size 0.05" for a PSF with FWHM 0.05"). -
2019 Product Guide ICE and OPEN WATER FISHING
2019 Product Guide ICE AND OPEN WATER FISHING ® ® S IT’S ® INK ALI T TH VE HE T WORM THA Flu Flu AMERICA’S PREMIER rippinlips.net PANFISH LURE Our Mission From humble basement beginnings nearly 30 years ago, Custom Jigs & Spins is still a family-run company with the same Table Of Contents simple mission – build high-quality jigs & tackle that catches fish. Custom Jigs & Spins Tackle B-Fish-N Tackle 2-3 . RPM - Rotating Power Minnow 33 . H2O Precision Jig 4-7 . Top Tungsten Ice Jigs: Chekai, Majmün, 34 . Draggin’ Jig & “Bucktail” Wayne’s Bucktail Jig JaJe and Glazba with Pro Panfish Picks 35 . MasterFlash Jig 8 . The Original Slender Spoon 37 . B3 Blade Bait 9 . Hammered Slender Spoon AuthentX Plastic Series & PFDC - Pro Finesse Drop Chain 39 . Moxi 10 . Pro Series Slender Spoon 40-41 . Pulse-R Paddletail 11 . Pro-Glow Series Slender Spoon 43 . Ribb-Finn 13 . The Original Demon 45 . 4” Ringworm 14 . Mega Glow Demon & Demon Perch Eye 6 46 . 3 .25” Paddletail 15 . Demon Jigging Spoon 47 . 5” K-Grub 16 . Slip Dropper System The Worm Tackle 17 . 2-Spot 48-49 . The Worm Pre-Rig 18 . Rocker 19 . Striper Special Rippin’ Lips Tackle 21 . ’Gill Pill & Diamond Jig 50-51 . SuperCat Rods 22 . Purest 53 . Tournament Grade Circle Hooks 23 . Ratfinkee 54 . Bootleg Dip Bait 24 . Ratso 55 . Big Fish Gripper 25 . Shrimpo 56 . Scent Trail & No Trace 26 . Pro Microplastics: Original Finesse Plastic Accessories plus Noodel & Micro Noodel 57 . Decals for Your Truck or Boat 27 . Nuclear Ant 58-59 . Rose Creek Polar Boxes, CJS Lure Boxes, Nuclear Flash 28 . -
Inertial Taylor Columns M D Jupiter's Great Red Spot1
744 JOURNAL OF THE ATMOSPHERIC SClESCES VOLUME26 Inertial Taylor Columns md Jupiter's Great Red Spot1 Division of Geological Sciences, California Institute of Teclznology, Pasadena (Manuscript received 18 July 1968, in revised form 4 February 1969) ABSTRACT A homogeneous fluid is bounded above and below by horizontal plane surfaces in rapid rotation about a vertical axis. An obstacle is attached to one of the surfaces, and at large distances from the obstacle the relative velocity is steady and horizontal. Solutions are obtained as power series expansions in the Rossby number, uniformly valid as the Taylor number approaches infinity. If the height of the obstacle is greater than the Rossby number times the depth, a stagnant region (Taylor column) forms over the obstacle. Outside this region there is a net circulation in a direction opposite the rotation. The shape of the stagnant region and the circulation are uniquely determined as part of the solution. Possible geophysical applications are discussed, and it is shown that stratification renders Taylor columns unlikely on earth, but that the Great Red Spot of Jupiter may be an example of this phenomenon, as Hide has suggested. 1. Introduction symmetric obstacle attached to one plane. The fluid within the Taylor column is found to be stagnant, Taylor (1917) and Proudman (1916) first showed that and the streamlines are symmetric to the left and right steady, weak currents in a rotating homogeneous fluid of the obstacle, as well as upstream and downstream are two-dimensional : the fluid moves about in columns from it. Jacobs' solution emphasizes the importance of whose axes are parallel to the rotation vector. -
SPITZER SPACE TELESCOPE MID-IR LIGHT CURVES of NEPTUNE John Stauffer1, Mark S
The Astronomical Journal, 152:142 (8pp), 2016 November doi:10.3847/0004-6256/152/5/142 © 2016. The American Astronomical Society. All rights reserved. SPITZER SPACE TELESCOPE MID-IR LIGHT CURVES OF NEPTUNE John Stauffer1, Mark S. Marley2, John E. Gizis3, Luisa Rebull1,4, Sean J. Carey1, Jessica Krick1, James G. Ingalls1, Patrick Lowrance1, William Glaccum1, J. Davy Kirkpatrick5, Amy A. Simon6, and Michael H. Wong7 1 Spitzer Science Center (SSC), California Institute of Technology, Pasadena, CA 91125, USA 2 NASA Ames Research Center, Space Sciences and Astrobiology Division, MS245-3, Moffett Field, CA 94035, USA 3 Department of Physics and Astronomy, University of Delaware, Newark, DE 19716, USA 4 Infrared Science Archive (IRSA), 1200 E. California Boulevard, MS 314-6, California Institute of Technology, Pasadena, CA 91125, USA 5 Infrared Processing and Analysis Center, MS 100-22, California Institute of Technology, Pasadena, CA 91125, USA 6 NASA Goddard Space Flight Center, Solar System Exploration Division (690.0), 8800 Greenbelt Road, Greenbelt, MD 20771, USA 7 University of California, Department of Astronomy, Berkeley CA 94720-3411, USA Received 2016 July 13; revised 2016 August 12; accepted 2016 August 15; published 2016 October 27 ABSTRACT We have used the Spitzer Space Telescope in 2016 February to obtain high cadence, high signal-to-noise, 17 hr duration light curves of Neptune at 3.6 and 4.5 μm. The light curve duration was chosen to correspond to the rotation period of Neptune. Both light curves are slowly varying with time, with full amplitudes of 1.1 mag at 3.6 μm and 0.6 mag at 4.5 μm. -
Mercury Friday, February 23
ASTRONOMY 161 Introduction to Solar System Astronomy Class 18 Mercury Friday, February 23 Mercury: Basic characteristics Mass = 3.302×1023 kg (0.055 Earth) Radius = 2,440 km (0.383 Earth) Density = 5,427 kg/m³ Sidereal rotation period = 58.6462 d Albedo = 0.11 (Earth = 0.39) Average distance from Sun = 0.387 A.U. Mercury: Key Concepts (1) Mercury has a 3-to-2 spin-orbit coupling (not synchronous rotation). (2) Mercury has no permanent atmosphere because it is too hot. (3) Like the Moon, Mercury has cratered highlands and smooth plains. (4) Mercury has an extremely large iron-rich core. (1) Mercury has a 3-to-2 spin-orbit coupling (not synchronous rotation). Mercury is hard to observe from the Earth (because it is so close to the Sun). Its rotation speed can be found from Doppler shift of radar signals. Mercury’s unusual orbit Orbital period = 87.969 days Rotation period = 58.646 days = (2/3) x 87.969 days Mercury is NOT in synchronous rotation (1 rotation per orbit). Instead, it has 3-to-2 spin-orbit coupling (3 rotations for 2 orbits). Synchronous rotation (WRONG!) 3-to-2 spin-orbit coupling (RIGHT!) Time between one noon and the next is 176 days. Sun is above the horizon for 88 days at the time. Daytime temperatures reach as high as: 700 Kelvin (800 degrees F). Nighttime temperatures drops as low as: 100 Kelvin (-270 degrees F). (2) Mercury has no permanent atmosphere because it is too hot (and has low escape speed). Temperature is a measure of the 3kT v = random speed of m atoms (or v typical speed of atom molecules). -
How to Calculate Planetary-Rotation Periods
Explaining Planetary-Rotation Periods Using an Inductive Method Gizachew Tiruneh, Ph. D., Department of Political Science, University of Central Arkansas (First submitted on June 19th, 2009; last updated on June 15th, 2011) This paper uses an inductive method to investigate the factors responsible for variations in planetary-rotation periods. I began by showing the presence of a correlation between the masses of planets and their rotation periods. Then I tested the impact of planetary radius, acceleration, velocity, and torque on rotation periods. I found that velocity, acceleration, and radius are the most important factors in explaining rotation periods. The effect of mass may be rather on influencing the size of the radii of planets. That is, the larger the mass of a planet, the larger its radius. Moreover, mass does also influence the strength of the rotational force, torque, which may have played a major role in setting the initial constant speeds of planetary rotation. Key words: Solar system; Planet formation; Planet rotation Many astronomers believe that planetary rotation is influenced by angular momentum and related phenomena, which may have occurred during the formation of the solar system (Alfven, 1976; Safronov, 1995; Artemev and Radzievskii, 1995; Seeds, 2001; Balbus, 2003). There is, however, not much identifiable recent research on planetary-rotation periods. Hughes’ (2003) review of the literature reveals that much research is needed to understand the phenomenon of planetary spin. Some of the assumptions that scholars have made in the past, according to Hughes (2003), include that planetary spin is a function of the gaseous or terrestrial nature of planets, that there is a power law relationship between planetary spin angular momentum and planetary mass, that there is a relationship between planets’ escape velocities and their spin rates, and that mass-independent spin periods can be obtained if one posits that a planetary formation process is governed by the balance between gravitational and centrifugal forces at the planetary equator. -
Determining the Rotation Period of the Sun
SOLAR PHYSICS AND TERRESTRIAL EFFECTS 2+ Activity 8 4= Activity 8 Determining the Rotation Period of the Sun Relevant Reading Chapter 2, section 3 Purpose Determine the rotation period of the Sun. Although numerous methods for accurate measurement are used in solar research, the method described here, using photographs taken over several days, will allow determination to within an Earth-day. Materials Photo set that shows at least one solar feature that can be followed over a several-day period. For real challenge, take the photos yourself, or make a simple projection sketch of sunspots over several days. 1 sheet of clear plastic used for overhead transparencies or viewgraphs, or something similar such as a clear plastic report folder a mm ruler, compass and protractor a fine-tipped marking pen suitable for plastic graph paper with 1-mm squares Procedures 1. Measure, to the nearest millimeter, the diameter of the Sun on the photo taken near the middle of the data period. 2. Use a compass and draw a circle with the same diameter on the transpar- ent sheet. 3. With the circle aligned over the photo on the date used for the diameter, trace the axis orientation marks onto the transparency. 4. Pick a solar feature that traverses the solar disk for as many days as pos- sible. Align the circle on the transparency over each successive photo and carefully mark the position of the chosen solar feature along with its date. 5. Carefully draw the best fitting straight line through the marked positions and measure its length across the circle as accurately as possible.