A Solar System Adventure General Information Imagine It
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JUICE Red Book
ESA/SRE(2014)1 September 2014 JUICE JUpiter ICy moons Explorer Exploring the emergence of habitable worlds around gas giants Definition Study Report European Space Agency 1 This page left intentionally blank 2 Mission Description Jupiter Icy Moons Explorer Key science goals The emergence of habitable worlds around gas giants Characterise Ganymede, Europa and Callisto as planetary objects and potential habitats Explore the Jupiter system as an archetype for gas giants Payload Ten instruments Laser Altimeter Radio Science Experiment Ice Penetrating Radar Visible-Infrared Hyperspectral Imaging Spectrometer Ultraviolet Imaging Spectrograph Imaging System Magnetometer Particle Package Submillimetre Wave Instrument Radio and Plasma Wave Instrument Overall mission profile 06/2022 - Launch by Ariane-5 ECA + EVEE Cruise 01/2030 - Jupiter orbit insertion Jupiter tour Transfer to Callisto (11 months) Europa phase: 2 Europa and 3 Callisto flybys (1 month) Jupiter High Latitude Phase: 9 Callisto flybys (9 months) Transfer to Ganymede (11 months) 09/2032 – Ganymede orbit insertion Ganymede tour Elliptical and high altitude circular phases (5 months) Low altitude (500 km) circular orbit (4 months) 06/2033 – End of nominal mission Spacecraft 3-axis stabilised Power: solar panels: ~900 W HGA: ~3 m, body fixed X and Ka bands Downlink ≥ 1.4 Gbit/day High Δv capability (2700 m/s) Radiation tolerance: 50 krad at equipment level Dry mass: ~1800 kg Ground TM stations ESTRAC network Key mission drivers Radiation tolerance and technology Power budget and solar arrays challenges Mass budget Responsibilities ESA: manufacturing, launch, operations of the spacecraft and data archiving PI Teams: science payload provision, operations, and data analysis 3 Foreword The JUICE (JUpiter ICy moon Explorer) mission, selected by ESA in May 2012 to be the first large mission within the Cosmic Vision Program 2015–2025, will provide the most comprehensive exploration to date of the Jovian system in all its complexity, with particular emphasis on Ganymede as a planetary body and potential habitat. -
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. -
The Solar System Cause Impact Craters
ASTRONOMY 161 Introduction to Solar System Astronomy Class 12 Solar System Survey Monday, February 5 Key Concepts (1) The terrestrial planets are made primarily of rock and metal. (2) The Jovian planets are made primarily of hydrogen and helium. (3) Moons (a.k.a. satellites) orbit the planets; some moons are large. (4) Asteroids, meteoroids, comets, and Kuiper Belt objects orbit the Sun. (5) Collision between objects in the Solar System cause impact craters. Family portrait of the Solar System: Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, Neptune, (Eris, Ceres, Pluto): My Very Excellent Mother Just Served Us Nine (Extra Cheese Pizzas). The Solar System: List of Ingredients Ingredient Percent of total mass Sun 99.8% Jupiter 0.1% other planets 0.05% everything else 0.05% The Sun dominates the Solar System Jupiter dominates the planets Object Mass Object Mass 1) Sun 330,000 2) Jupiter 320 10) Ganymede 0.025 3) Saturn 95 11) Titan 0.023 4) Neptune 17 12) Callisto 0.018 5) Uranus 15 13) Io 0.015 6) Earth 1.0 14) Moon 0.012 7) Venus 0.82 15) Europa 0.008 8) Mars 0.11 16) Triton 0.004 9) Mercury 0.055 17) Pluto 0.002 A few words about the Sun. The Sun is a large sphere of gas (mostly H, He – hydrogen and helium). The Sun shines because it is hot (T = 5,800 K). The Sun remains hot because it is powered by fusion of hydrogen to helium (H-bomb). (1) The terrestrial planets are made primarily of rock and metal. -
Planetary Rings
CLBE001-ESS2E November 10, 2006 21:56 100-C 25-C 50-C 75-C C+M 50-C+M C+Y 50-C+Y M+Y 50-M+Y 100-M 25-M 50-M 75-M 100-Y 25-Y 50-Y 75-Y 100-K 25-K 25-19-19 50-K 50-40-40 75-K 75-64-64 Planetary Rings Carolyn C. Porco Space Science Institute Boulder, Colorado Douglas P. Hamilton University of Maryland College Park, Maryland CHAPTER 27 1. Introduction 5. Ring Origins 2. Sources of Information 6. Prospects for the Future 3. Overview of Ring Structure Bibliography 4. Ring Processes 1. Introduction houses, from coalescing under their own gravity into larger bodies. Rings are arranged around planets in strikingly dif- Planetary rings are those strikingly flat and circular ap- ferent ways despite the similar underlying physical pro- pendages embracing all the giant planets in the outer Solar cesses that govern them. Gravitational tugs from satellites System: Jupiter, Saturn, Uranus, and Neptune. Like their account for some of the structure of densely-packed mas- cousins, the spiral galaxies, they are formed of many bod- sive rings [see Solar System Dynamics: Regular and ies, independently orbiting in a central gravitational field. Chaotic Motion], while nongravitational effects, includ- Rings also share many characteristics with, and offer in- ing solar radiation pressure and electromagnetic forces, valuable insights into, flattened systems of gas and collid- dominate the dynamics of the fainter and more diffuse dusty ing debris that ultimately form solar systems. Ring systems rings. Spacecraft flybys of all of the giant planets and, more are accessible laboratories capable of providing clues about recently, orbiters at Jupiter and Saturn, have revolutionized processes important in these circumstellar disks, structures our understanding of planetary rings. -
The Search for Exomoons and the Characterization of Exoplanet Atmospheres
Corso di Laurea Specialistica in Astronomia e Astrofisica The search for exomoons and the characterization of exoplanet atmospheres Relatore interno : dott. Alessandro Melchiorri Relatore esterno : dott.ssa Giovanna Tinetti Candidato: Giammarco Campanella Anno Accademico 2008/2009 The search for exomoons and the characterization of exoplanet atmospheres Giammarco Campanella Dipartimento di Fisica Università degli studi di Roma “La Sapienza” Associate at Department of Physics & Astronomy University College London A thesis submitted for the MSc Degree in Astronomy and Astrophysics September 4th, 2009 Università degli Studi di Roma ―La Sapienza‖ Abstract THE SEARCH FOR EXOMOONS AND THE CHARACTERIZATION OF EXOPLANET ATMOSPHERES by Giammarco Campanella Since planets were first discovered outside our own Solar System in 1992 (around a pulsar) and in 1995 (around a main sequence star), extrasolar planet studies have become one of the most dynamic research fields in astronomy. Our knowledge of extrasolar planets has grown exponentially, from our understanding of their formation and evolution to the development of different methods to detect them. Now that more than 370 exoplanets have been discovered, focus has moved from finding planets to characterise these alien worlds. As well as detecting the atmospheres of these exoplanets, part of the characterisation process undoubtedly involves the search for extrasolar moons. The structure of the thesis is as follows. In Chapter 1 an historical background is provided and some general aspects about ongoing situation in the research field of extrasolar planets are shown. In Chapter 2, various detection techniques such as radial velocity, microlensing, astrometry, circumstellar disks, pulsar timing and magnetospheric emission are described. A special emphasis is given to the transit photometry technique and to the two already operational transit space missions, CoRoT and Kepler. -
Lesson -14 the Outer Space
Lesson -14 The Outer Space Q1. Fill in the blanks: 1. The moon rotates around the earth. 2. A group of stars is called constellation. 3. Moon is the natural satellite of earth. 4. When we cannot see the moon in the sky, it is called amavasya. 5. The sun is a star. Q2. Choose the correct answer: 1. Huge glowing balls of fire are called___________. a) Satellites b) sun 2. The moon rotates around the _____________. a) Earth b) Mars 3. A group of stars forms a ___________. a) Satellite b) constellation 4. We can see full moon on ___________. a) Amavasya b) purnima 5. The moon gets its light from the _____________. a) Earth b) sun Q3. True or False: 1. Stars go away from the sky during the day – False. 2. Moon gets its light from earth –False. 3. We can live on moon –False. 4. Earth is the first planet from the sun – False. 5. Sun gives us heat and light – True. Q4. Match the following: 1. Sun - dwarf planet (5) 2. Moon - constellation (4) 3. Earth - satellite (2) 4. Leo - star (1) 5. Pluto - third planet from sun ( 3) Q5. Give two examples each of: 1. Heavenly bodies: Ans: (i) Moon (ii) planets. 2. Planets: Ans: (i) Earth (ii) mars 3. Stars: Ans: (i) Sun (ii) pole star 4. Constellations: Ans: (i) orion (ii) Leo 5. Satellites: Ans: (i) moon (ii)Earth Q6. Short answer: 1. What does the universe consist of? Ans: The universe consists of heavenly bodies like stars, planets and moon. 2. -
Orbital Dynamics and Numerical N-Body Simulations of Extrasolar Moons and Giant Planets
ORBITAL DYNAMICS AND NUMERICAL N-BODY SIMULATIONS OF EXTRASOLAR MOONS AND GIANT PLANETS. A Dissertation Presented to the Faculty of the Graduate School of Cornell University in Partial Fulfillment of the Requirements for the Degree of Doctor of Philosophy by Yu-Cian Hong August 2019 c 2019 Yu-Cian Hong ALL RIGHTS RESERVED ORBITAL DYNAMICS AND NUMERICAL N-BODY SIMULATIONS OF EXTRASOLAR MOONS AND GIANT PLANETS. Yu-Cian Hong, Ph.D. Cornell University 2019 This thesis work focuses on computational orbital dynamics of exomoons and exoplanets. Exomoons are highly sought-after astrobiological targets. Two can- didates have been discovered to-date (Bennett et al., 2014, Teachey & Kipping, 2018). We developed the first N-body integrator that can handle exomoon orbits in close planet-planet interactions, for the following three projects. (1) Instability of moons around non-oblate planets associated with slowed nodal precession and resonances with stars.This work reversed the commonsensical notion that spinning giant planets should be oblate. Moons around spherical planets were destabilized by 3:2 and 1:1 resonance overlap or the chaotic zone around 1:1 resonance between the orbital precession of the moons and the star. Normally, the torque from planet oblateness keeps the orbit of close-in moons precess fast ( period ∼ 7 yr for Io). Without planet oblateness, Io?s precession period is much longer (∼ 104 yr), which allowed resonance with the star, thus the in- stability. Therefore, realistic treatment of planet oblateness is critical in moon dynamics. (2) Orbital stability of moons in planet-planet scattering. Planet- planet scattering is the best model to date for explaining the eccentricity distri- bution of exoplanets. -
Natural Satellite Background I: the Gravitational
Stuart Greenbaum: Natural Satellite Analysis by the composer Background In 2013, I was approached by the Classical Guitar Society of Victoria to write a new work for Slava and Leonard Grigoryan. I had an idea to write a piece about moons; and in the ensuing discussions it was mooted that perhaps we could therefore premiere the work at the Melbourne Planetarium. We were put in touch with Dr Tanya Hill, who was very supportive of the idea and creating visuals in the Planetarium dome at Scienceworks to match the with five movements DigitalSky Programming. It was subsequently premiered on 15 November 2013 at Melbourne Planetarium (two shows), repeated on 16 February 2014, and then given a two further concert performances at the Melbourne Recital Centre on 17 April 2014. A natural satellite, moon, or secondary planet is a celestial body that orbits a planet or smaller body, which is called its primary. Earth has one large natural s satellite, known a the Moon. No "moons of moons" (natural satellites that orbit the natural satellite of another body) are known. In most cases, the tidal effects of the primary would make such a system unstable. The seven largest natural satellites in the Solar System are Jupiter's Galilean moons (Ganymede, Callisto, Io, and Europa), Saturn's moon Titan, Earth's Moon, and Neptune's captured natural satellite Triton. I: The gravitational influence of Titan Most regular moons in the Solar System are tidally locked to their respective primaries, meaning that the same side of the natural satellite always faces its planet. -
Stellium Handbook Part
2 Donna Cunningham’s Books on the Outer Planets If you’re dealing with a stellium that contains one or more outer planets, these ebooks will help you understand their role in your chart and explore ways to change difficult patterns they represent. Since The Stellium Handbook can’t cover them in the depth they deserve, you’ll gain a greater perspective through these ebooks that devote entire chapters to the meanings of Uranus, Neptune, or Pluto in a variety of contexts. The Outer Planets and Inner Life volumes are $15 each if purchased separately, or $35 for all three—a $10 savings. To order, go to PayPal.com and tell them which books you want, Donna’s email address ([email protected]), and the amount. The ebooks arrive on separate emails. If you want them sent to an email address other than the one you used, let her know. The Outer Planets and Inner Life, V.1: The Outer Planets as Career Indicators. If your stellium has outer planets in the career houses (2nd, 6th, or 10th), or if it relates to your chosen career, this book can give you helpful insights. There’s an otherworldly element when the outer planets are career markers, a sense of serving a greater purpose in human history. Each chapter of this e-book explores one of these planets in depth. See an excerpt here. The Outer Planets and Inner Life, v.2: Outer Planet Aspects to Venus and Mars. Learn about the love lives of people who have the outer planets woven in with the primary relationship planets, Venus and Mars, or in the relationship houses—the 7th, 8th, and 5th. -
Roving on Phobos: Challenges of the Mmx Rover for Space Robotics
View metadata, citation and similar papers at core.ac.uk brought to you by CORE provided by Institute of Transport Research:Publications ROVING ON PHOBOS: CHALLENGES OF THE MMX ROVER FOR SPACE ROBOTICS Jean Bertrand (1), Simon Tardivel (1), Frans IJpelaan (1), Emile Remetean (1), Alex Torres (1), Stéphane Mary (1), Maxime Chalon (2), Fabian Buse (2), Thomas Obermeier (2), Michal Smisek (2), Armin Wedler (2), Joseph Reill (2), Markus Grebenstein (2) (1) CNES, 18 avenue Edouard Belin 31401 Toulouse Cedex 9 (France), [email protected] (2) DLR, Münchener Straße 20 82234 Weßling (Germany), [email protected] ABSTRACT Once on the surface, the rover would deploy and upright itself from its stowed position and orientation, and carry This paper presents a small rover for exploration mission out several science objectives over the course of a few dedicated to the moons of Mars, Phobos and Deimos. months. In October 2018, CNES and DLR have This project is a collaboration between JAXA for the expressed their interest in partnering together on this mother spacecraft, and a cooperative contribution of project and the MMX rover is now a joint project of both CNES and DLR to provide a rover payload. organizations in tight cooperation. After a description of the MMX mission defined by JAXA, this paper presents This rover will be different in many aspects compared to the Phobos environment. Then, it details the mission the existing ones. It will have to drive in a very low constraints and the rover objectives. It outlines some gravity with only little power given by the solar arrays. -
Resonant Moons of Neptune
EPSC Abstracts Vol. 13, EPSC-DPS2019-901-1, 2019 EPSC-DPS Joint Meeting 2019 c Author(s) 2019. CC Attribution 4.0 license. Resonant moons of Neptune Marina Brozović (1), Mark R. Showalter (2), Robert A. Jacobson (1), Robert S. French (2), Jack L. Lissauer (3), Imke de Pater (4) (1) Jet Propulsion Laboratory, California Institute of Technology, California, USA, (2) SETI Institute, California, USA, (3) NASA Ames Research Center, California, USA, (4) University of California Berkeley, California, USA Abstract We used integrated orbits to fit astrometric data of the 2. Methods regular moons of Neptune. We found a 73:69 inclination resonance between Naiad and Thalassa, the 2.1 Observations two innermost moons. Their resonant argument librates around 180° with an average amplitude of The astrometric data cover the period from 1981-2016, ~66° and a period of ~1.9 years. This is the first fourth- with the most significant amount of data originating order resonance discovered between the moons of the from the Voyager 2 spacecraft and HST. Voyager 2 outer planets. The resonance enabled an estimate of imaged all regular satellites except Hippocamp the GMs for Naiad and Thalassa, GMN= between 1989 June 7 and 1989 August 24. The follow- 3 -2 3 0.0080±0.0043 km s and GMT=0.0236±0.0064 km up observations originated from several Earth-based s-2. More high-precision astrometry of Naiad and telescopes, but the majority were still obtained by HST. Thalassa will help better constrain their masses. The [4] published the latest set of the HST astrometry GMs of Despina, Galatea, and Larissa are more including the discovery and follow up observations of difficult to measure because they are not in any direct Hippocamp.