{TEXTBOOK} Phobos

Total Page:16

File Type:pdf, Size:1020Kb

{TEXTBOOK} Phobos PHOBOS PDF, EPUB, EBOOK Eddie Robson, Paul McGann, Sheridan Smith | none | 30 May 2007 | Big Finish Productions Ltd | 9781844352593 | English | Maidenhead, United Kingdom Phobos on Steam There is certainly evidence that Phobos has suffered the occasional asteroid impact. Given that Phobos is so small, there is another potential source for impact debris on its surface. Such debris might actually be flung at Phobos from the surface of Mars, as the Red Planet is hit by asteroids from time to time. Some computations suggest about parts per million — or even more — of the unconsolidated rock debris on Phobos's surface came from Mars. Alternatively, the Phobos monolith might not have formed during an impact. It could be a rare chunk of the moon's solid bedrock, poking up through a surface that is otherwise mostly strewn with loose debris. This is an idea that was discussed several years ago by planetary scientists exploring the possibility of a mission to Phobos. If this hypothesis is true, it would mean the monolith could hold clues about the origins of Phobos itself. And that would make the monolith a surprisingly big deal. According to some planetary science, Phobos is just about the most mysterious body in the known Solar System. Phobos is one of two tiny moons orbiting Mars, the other being Deimos. It is not really clear how they got there. Both are small and irregular in shape, which makes them look a little like asteroids that fell into Mars's gravitational clutches long ago. But the moons orbit Mars in a way that is incompatible with this "snatched asteroid" idea. Eventually, the large moon and all but two of the small moons orbited so close to Mars that they disintegrated. An alternative is that they formed from the same material that Mars did when the planet coalesced billions of years ago. However, precise astronomical measurements reveal that Phobos has a much lower density than typical Martian rock. That leaves a third idea: Mars suffered a devastating impact with a large protoplanet long ago, which generated the two moons. A similar sort of collision is thought to be behind the creation of Earth's Moon. But our Moon is large, and Phobos and Deimos are tiny. A massive impact should have given Mars a much larger satellite. They both conclude that the third idea is correct. While one adds further evidence that the moons are not captured asteroids , the second sets out a detailed scenario that can explain how Mars ended up with two tiny moons. The massive impact did, apparently, generate a large moon. It was this large moon that encouraged the formation of Phobos and Deimos, and several other satellites, from the leftover debris. Eventually, the large moon and all but two of the small moons orbited so close to Mars that they disintegrated and returned to the Martian surface. Phobos and Deimos alone survive. Proposed expeditions to analyse the composition of Phobos , and its monolith, could test this idea. But the clock is ticking. By continuing to use the site you are agreeing to our use of cookies. OK Find out more about our cookie policy. Toggle navigation Toggle navigation. Toggle mission navigation. Missions Show All Missions. Asset Publisher Martian moons: Phobos. Martian moons: Phobos. Video is not supported. Images And Videos. Images And Videos Deimos. Mars- facing side of Phobos. Close-up of Phobos, acquired on 28 July Phobos and Deimos. Pioneering images of both Martian moons. Orbits of Mars Express and the Martian moons. Phobos Related Publications. Rosenblatt, P. Related Publications Rosenblatt, P. Related Links. See Also. Mars Express to make closest ever approach to Phobos. See Also Mars Express to make closest ever approach to Phobos. All rights reserved. Terms and Conditions. An image of the Mars-facing side of Phobos. Key parameters for Phobos. phobos - Перевод на русский - примеры английский | Reverso Context Measurements of the day and night sides of Phobos show such extreme temperature variations that the sunlit side of the moon rivals a pleasant winter day in Chicago, while only a few kilometers away, on the dark side of the moon, the climate is more harsh than a night in Antarctica. High temperatures for Phobos were measured at 25 degrees Fahrenheit -4 degrees Celsius and lows at degrees Fahrenheit degrees Celsius. This intense heat loss is likely a result of the fine dust on Phobos' surface, which is unable to retain heat. Phobos has no atmosphere. It may be a captured asteroid, but some scientists show evidence that contradicts this theory. Hall named Mars' moons for the mythological sons of Ares, the Greek counterpart of the Roman god, Mars. Phobos, whose name means fear is the brother of Deimos. Overview Phobos, gouged and nearly shattered by a giant impact crater and beaten by thousands of meteorite impacts, is on a collision course with Mars. A 3D model of Phobos, on of two moons of Mars. In Depth. The symbols, mottos, and small objects added to the agency's newest Mars rover serve a variety of purposes, from functional to decorative. NASA's Perseverance rover carries a device to convert Martian air into oxygen that one day could be used not just for breathing, but also for fuel. The first rover to be rigged with microphones, Perseverance picked up sounds of its inner workings during flight. Plumes of water vapor that may be venting into space from Jupiter's moon Europa could come from within the icy crust itself, according to new research. This latest is from a location named "Mary Anning," after a 19th-century English paleontologist. Mark your calendars: NASA's latest rover has only about days to go before it touches down on the Red Planet, becoming history's next Mars car. New experiments re-create the environment of Europa and find that the icy moon shines, even on its nightside. The effect is more than just a cool visual. The next full Moon will be on the morning of Halloween, Saturday, Oct. Perseverance has about million miles million kilometers left to reach its destination. This illustration shows Jezero Crater — the landing site of the Mars Perseverance rover — as it may have looked billions of years ago. Remarkable linear grooves, typically metres feet wide and 20 metres 65 feet deep, cover much of the surface. There is strong evidence that they are associated with the formation of the largest crater on Phobos. This structure, known as Stickney , measures about 10 km 6 miles across. If such is the case, it will collide with Mars in the very distant future. Phobos Article Media Additional Info. Home Science Astronomy. Print Cite. Facebook Twitter. Give Feedback External Websites. Let us know if you have suggestions to improve this article requires login. External Websites. NASA - Phobos. The Editors of Encyclopaedia Britannica Encyclopaedia Britannica's editors oversee subject areas in which they have extensive knowledge, whether from years of experience gained by working on that content or via study for an advanced degree See Article History. Video of Phobos's rotation as assembled from still photographs taken by the European Space Agency's Mars Express orbiter. Britannica Quiz. But how much do you know about the moons of other planets? BBC - Earth - There is a huge 'monolith' on Phobos, one of Mars's moons Science News. An image taken on February 25, , shows Phobos while in eclipse, where Mars' shadow completely blocked sunlight from reaching the moon's surface. This event resulted in some of the coldest temperatures measured on Phobos to date, with the coldest being about degrees Fahrenheit degrees Celsius. On March 27, , Phobos was observed exiting an eclipse, when its surface was still warming up. Related Multimedia : Images capture the Mars moon Phobos during different phases -- waxing, waning and full. ScienceDaily, 3 June Northern Arizona University. Origin of Martian moon Phobos. Retrieved December 14, from www. This dark aspect inspired the hypothesis that the close- orbiting moon may be a captured asteroid, but its Who put that there? These are the words of Buzz Aldrin, the second man to walk on the Moon, in He was talking about a peculiar and solitary large rock, a monolith, that sits on the surface of the Martian moon Phobos. Aldrin was right: many people are vexed by the Phobos monolith. It has inspired all manner of alien-based conspiracy theories and this fascinating discussion on Reddit. The monolith appears to be a large boulder, variously described as building-sized or 90m tall. It stands in a desolate, featureless region of Phobos, which probably makes the monolith seem even more impressive. Other spooky features, like the infamous face on Mars, do not seem quite so unusual when you take a closer look. It is not alone. Mars boasts a monolith of its own. However, the scientific community does not see such monoliths as evidence of advanced alien civilisations. The Martian monolith is almost certainly no more than a roughly straight-edged chunk of rock that tumbled down from a nearby cliff. Perfectly natural erosional forces can also explain why Mars seems to be home to a levitating spoon and an Egyptian-style pyramid. Other spooky features, like the infamous face on Mars , do not seem quite so unusual when you take a closer look or view them from a different angle. It is possibly simply a shard formed during an impact event. There is certainly evidence that Phobos has suffered the occasional asteroid impact. Given that Phobos is so small, there is another potential source for impact debris on its surface. Such debris might actually be flung at Phobos from the surface of Mars, as the Red Planet is hit by asteroids from time to time.
Recommended publications
  • Phobos, Deimos: Formation and Evolution Alex Soumbatov-Gur
    Phobos, Deimos: Formation and Evolution Alex Soumbatov-Gur To cite this version: Alex Soumbatov-Gur. Phobos, Deimos: Formation and Evolution. [Research Report] Karpov institute of physical chemistry. 2019. hal-02147461 HAL Id: hal-02147461 https://hal.archives-ouvertes.fr/hal-02147461 Submitted on 4 Jun 2019 HAL is a multi-disciplinary open access L’archive ouverte pluridisciplinaire HAL, est archive for the deposit and dissemination of sci- destinée au dépôt et à la diffusion de documents entific research documents, whether they are pub- scientifiques de niveau recherche, publiés ou non, lished or not. The documents may come from émanant des établissements d’enseignement et de teaching and research institutions in France or recherche français ou étrangers, des laboratoires abroad, or from public or private research centers. publics ou privés. Phobos, Deimos: Formation and Evolution Alex Soumbatov-Gur The moons are confirmed to be ejected parts of Mars’ crust. After explosive throwing out as cone-like rocks they plastically evolved with density decays and materials transformations. Their expansion evolutions were accompanied by global ruptures and small scale rock ejections with concurrent crater formations. The scenario reconciles orbital and physical parameters of the moons. It coherently explains dozens of their properties including spectra, appearances, size differences, crater locations, fracture symmetries, orbits, evolution trends, geologic activity, Phobos’ grooves, mechanism of their origin, etc. The ejective approach is also discussed in the context of observational data on near-Earth asteroids, main belt asteroids Steins, Vesta, and Mars. The approach incorporates known fission mechanism of formation of miniature asteroids, logically accounts for its outliers, and naturally explains formations of small celestial bodies of various sizes.
    [Show full text]
  • Download This PDF File
    Journal of Physics Special Topics P3_5 ALL THESE WORLDS ARE YOURS J. Bettles, I. Clarke, M. Perry and N. Pilkington. Department of Physics and Astronomy, University of Leicester, Leicester, LE1 7RH. November 03, 2011 Abstract This paper investigates a plot point of the novel 2010: Odyssey Two by Arthur C. Clarke in which self replicating monoliths engulf Jupiter, increasing its density to the point when nuclear fusion can take place, giving birth to a new star. It was found that 1.629x1020 monoliths would be needed to trigger nuclear fusion in Jupiter's core, taking 136 hours to do so. Mission Profile Anomaly 1) was stated as being 11 feet tall In the second novel of Arthur C. Clarke's (3.35m) with dimensions in the exact ratio of Space Odyssey series, 2010: Odyssey Two, a 1:4:9 (the squares of the first three integers) crew was sent to discover what went wrong for depth, width and height respectively [2]. with an earlier mission to investigate a The monolith found orbiting Jupiter, monolith (figure 1) in orbit around Jupiter. designated TMA-2 (doubly inaccurate since it Shortly after they arrived, the crew were told was neither discovered in the Tycho crater to leave as “something wonderful” was going nor did it give off any magnetic signal), had to happen. The monolith disappeared from dimensions in the exact same ratio, but was orbit and a dark spot appeared on Jupiter and 718 times bigger than TMA-1 [3]. This enabled began to grow. The spot was a population of us to calculate the dimensions of TMA-2 as monoliths that were self replicating 267.5x1070x2407m with a volume of exponentially and consuming the planet.
    [Show full text]
  • Mars, Phobos, and Deimos Sample Return Enabled by ARRM Alternative Trade Study Spacecraft
    Mars, Phobos, and Deimos Sample Return Enabled by ARRM Alternative Trade Study Spacecraft Jacob A. Englander,∗ Matthew A. Vavrina,† Bo Naasz ,‡ Raymond G. Merill,MinQu§ ¶ The Asteroid Robotic Redirect Mission (ARRM) has been the topic of many mission design studies since 2011.1 The reference ARRM spacecraft uses a powerful solar electric propulsion (SEP) system and a bag device to capture a small asteroid from an Earth-like orbit and redirect it to a distant retrograde orbit (DRO) around the moon. The ARRM Option B spacecraft uses the same propulsion system and multi-Degree of Freedom (DoF) manipulators device to retrieve a very large sample (thousands of kilograms) from a 100+ meter diameter farther-away Near Earth Asteroid (NEA). This study will demonstrate that the ARRM Option B spacecraft design can also be used to return samples from Mars and its moons - either by acquiring a large rock from the surface of Phobos or Deimos, and/or by rendezvousing with a sample-return spacecraft launched from the surface of Mars. I. Introduction The Asteroid Robotic Redirect Mission (ARRM) Option A concept, first introduced in 2011,1 is a mission design to capture and return a small near-Earth asteroid (NEA) to cislunar space. The ARRM Option B concept is a similar spacecraft, but designed to return a very large sample from a more difficult to reach NEA.2 In this work we show that the spacecraft designed for ARRM Option B is also well-suited to sample return from Mars and its moons. This work presents low-thrust interplanetary trajectories from cislunar space to Mars and back, including descent from the Martian sphere of influence (SOI) to the desired orbit altitude and ascent to the SOI after the sample retrieval is complete.
    [Show full text]
  • Deimos and Phobos As Destinations for Human Exploration
    Deimos and Phobos as Destinations for Human Exploration Josh Hopkins Space Exploration Architect Lockheed Martin Caltech Space Challenge March 2013 © 2013 Lockheed Martin Corporation. All Rights Reserved 1 Topics • Related Lockheed Martin mission studies • Orbital mechanics vs solar cycles • Relevant characteristics of Phobos and Deimos • Locations to land • Considerations for designing your mission • Suggested trades 2 Stepping Stones Stepping Stones is a series of exploration 2023 missions building incrementally towards Deimos Scout the long term goal of exploring Mars. Each mission addresses science objectives relating to the formation of the solar 2031-2035 system and the origins of life. Red Rocks: explore Mars from Deimos 2024, 2025, 2029 2017 Plymouth Rock: Humans explore asteroids like Asteroid scout 1999 AO10 and 2000 SG344 2018-2023 Fastnet: Explore the Moon’s far side from Earth-Moon L2 region 2016 Asteroid survey 2017 SLS test flight 2013-2020 Human systems tests on ISS Lockheed Martin Notional Concept Dates subject to change 3 Deimos photo courtesy of NASA-JPL, University of Arizona Summary • A human mission to one of the two moons of Mars would be an easier precursor to a mission to land on Mars itself. • Astronauts would explore the moon in person and teleoperate rovers on the surface of Mars with minimal lag time, with the goal of returning samples to Earth. • “Red Rocks” mission to land on a Martian moon would follow “Plymouth Rock” missions to a Near Earth Asteroid. • Comparison of Deimos and Phobos revealed Deimos is the preferred destination for this mission. • We identified specific areas on Deimos and Phobos as optimal landing sites for an early mission focused on teleoperation.
    [Show full text]
  • The Moon (~1700Km) an Asteroid (~50Km)
    1) inventory Solar System 2) spin/orbit/shape 3) heated by the Sun overview 4) how do we fnd out Inventory 1 star (99.9% of M) 8 planets (99.9% of L) - Terrestrial: Mercury Venus Earth Mars - Giant: Jupiter Saturn Uranus Neptune Lots of small bodies incl. dwarf planets Ceres Pluto Eris Maybe a 9th planet? Moons of Jupiter Inventory (cont'd) 4 Galilean satellites (Ganymede, Callisto, Io & Europa), 3 Many moons & rings ~10 km (close to Jupiter, likely primordial) Mercury: 0 Venus: 0 Earth: 1 (1700km) Mars: 2 (~10km) Jupiter: 69 + rings Saturn: 62 + rings Uranus: 27 + rings Neptune: 14 + rings 2001J3: 4km Even among dwarf planets, asteroids, Kuiper belt objects, and comets. E.g., Pluto: 5 Eris: 1 Moons of Mars: Deimos & Phobos, ~10km Atmosphere no thick thick little thick Inventory (cont'd) ~105 known small objects in the - Asteroid belt (Ceres ~300 km) - Kuiper belt (Eris, Pluto, Sedna, Quaoar, ~1000 km) Estimated: ~1012 comets in the - Oort cloud (~ 104 AU) Associated: - zodiacal dust (fre-works on the sky: comets & meteorites) What are planets? IAU (for solar system): Orbits Sun, massive enough to be round and to have cleared its neighbourhood. More general: 6 1) no nuclear fusion (not even deuterium): Tc < 10 K 2) pressure provided by electron degeneracy and/or Coulomb force (l ~ h/p ~ d) (d ~ atomic radius) 3) can be solid or gaseous (with solid cores) --- similar density Mass & Mean r M [g/cm3] R~M J Jupiter 1.0 1.33 R R~M1/3 Saturn 0.3 0.77 R~M-1/3 Neptune 0.05 1.67 Uranus 0.04 1.24 Earth 0.003 5.52 Venus 0.002 5.25 planets brown dwarfs stars Mars 0.0003 3.93 Mercury 0.0002 5.43 3 MJ 13 MJ 80 MJ M Orbits inclination: largely coplanar (history) direction: all the same eccentricity: a few percent (except for Mercury) Titus-Bode (ftting) law (1766) planetary orbits appear to (almost) satisfy a single relation 'Predict' the existence of the asteroid belt (1801: Ceres discovered) coincidence or something deeper? other systems? Computer simulations indicate that planets are as maximally packed as allowed by stability.
    [Show full text]
  • Phobos and Deimos CCD Observations,
    A&A 487, 755–758 (2008) Astronomy DOI: 10.1051/0004-6361:200809498 & c ESO 2008 Astrophysics Phobos and Deimos CCD observations, C. H. Veiga Observatório Nacional, Rua General José Cristino 77, Bairro Imperial de São Cristóvão Cep:20921-400 Rio de Janeiro, Brazil Coordenação de Astronomia e Astrofísica e-mail: [email protected] Received 1 February 2008 / Accepted 14 May 2008 ABSTRACT Aims. This paper give positions of Martian satellites system from CCD observations obtained at the Cassegrain focus of a 1.6 m reflector for the years 1995 and 2003. Methods. These positions were reduced using the scale and orientation parameters, determined from star field positions of Uranus and Pluto systems’ observations that were made in the same night as Mars observations. Results. They are compared with the theoretically calculated positions from JPL Development planetary Ephemeris – DE405. The standard deviations of the residuals, observed minus calculated positions, right ascension and declination of Phobos and Deimos, respectively are σ = 0. 079 and σ = 0. 072. Key words. celestial mechanics – astrometry – ephemerides 1. Introduction of 11.8 and 12.9, respectively, while the magnitude of the planet is −1.5, for two years observations, 1995 and 2003. Due to the The modern observations of the main planets and their satel- great difference in magnitude between them, and their orbits to lites are accomplished by spacecraft missions. These observa- be very close to the planet, 8.178 and 17.750 km, correspond- tions are important because the spacecraft flybys allow us to see ing to the mean distance for 1995 and 2003 missions, the strong the planet’s physical characteristics in greater detail.
    [Show full text]
  • 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
    [Show full text]
  • Solar System 3 Part Cards
    Sun Mercury Venus Earth Mars Jupiter Venus is the hottest planet in our solar Mercury is the planet closest to the sun. The sun is a star. It is the closest star system. The thick clouds on Venus It is the smallest of all the big planets. to Earth. hold the heat in. During the day on Mercury it gets very The sun is very hot. Its warmth and The sun’s lights reflect off Venus’s hot and at night it is very cold. light keep plants and animals alive on clouds making it look like the brightest Earth. star in the night sky. It takes only 88 days for Mercury to go around the sun. The sun is about 93 million miles away Venus is the closest planet to Earth. from Earth. Most of Venus is covered in lava and The sun is at the center of our solar volcanos. system. The planets in our solar Venus spins clockwise, the opposite system travel around the sun. It takes direction to Earth. 1 year or 365 days for the Earth to go around the sun. Venus spins slower than Earth. Jupiter is the biggest planet in our solar Mars is the most like Earth of all the Most of the Earth is covered with system. planets. oceans. Jupiter has a huge storm that’s been Mars has huge volcanoes. Earth is the 5th largest planet. blowing for hundreds of years called Mars has two small, funny shaped Earth has 1 moon. the Great Red Spot. moons called Phobos and Deimos.
    [Show full text]
  • The Crystal Monolith
    Firenze University Press www.fupress.com/substantia Feature Article 2001: The Crystal Monolith Citation: J.M. Garcia-Ruiz (2018) 2001: The Crystal Monolith. Substantia Juan Manuel Garcia-Ruiz 2(2): 19-25. doi: 10.13128/substantia- 57 Laboratorio de Estudios Cristalográficos. Instituto Andaluz de Ciencias de la Tierra. CSIC-Universidad de Granada. Spain Copyright: © 2018 J.M. Garcia-Ruiz. E-mail: [email protected] This is an open access, peer-reviewed article published by Firenze University Press (http://www.fupress.com/substan- Abstract. In the famous movie “2001: A Space Odyssey”, Stanley Kubrick and Arthur tia) and distribuited under the terms Clarke claim that an extraterrestrial civilization catalyzed the evolution of hominids of the Creative Commons Attribution on our planet. To represent such a powerful civilization, they use a crystal. To date, License, which permits unrestricted it seems that we have not been contacted by advanced civilizations and that we are use, distribution, and reproduction alone to manage our own future. Yet Kubrick and Clarke perhaps intuitively touched a in any medium, provided the original author and source are credited. truth about the power of crystals. An argument is developed here that genuine crystals, mainly quartz single crystals, were the earliest catalysts of the abstract thinking, sym- Data Availability Statement: All rel- bolism, and consciousness. evant data are within the paper and its Supporting Information files. Keywords. Crystals, crystallography, abstract thinking, paleoneurobiology, Kubrick, “2001: A Space Odissey”. Competing Interests: The Author(s) declare(s) no conflict of interest. THE MONOLITH OF “2001: A SPACE ODYSSEY” Art, in its very different forms, has contributed and contributes almost as much as science and philosophy to create our conception of the outside world.
    [Show full text]
  • Solar System Planet and Dwarf Planet Fact Sheet
    Solar System Planet and Dwarf Planet Fact Sheet The planets and dwarf planets are listed in their order from the Sun. Mercury The smallest planet in the Solar System. The closest planet to the Sun. Revolves the fastest around the Sun. It is 1,000 degrees Fahrenheit hotter on its daytime side than on its night time side. Venus The hottest planet. Average temperature: 864 F. Hotter than your oven at home. It is covered in clouds of sulfuric acid. It rains sulfuric acid on Venus which comes down as virga and does not reach the surface of the planet. Its atmosphere is mostly carbon dioxide (CO2). It has thousands of volcanoes. Most are dormant. But some might be active. Scientists are not sure. It rotates around its axis slower than it revolves around the Sun. That means that its day is longer than its year! This rotation is the slowest in the Solar System. Earth Lots of water! Mountains! Active volcanoes! Hurricanes! Earthquakes! Life! Us! Mars It is sometimes called the "red planet" because it is covered in iron oxide -- a substance that is the same as rust on our planet. It has the highest volcano -- Olympus Mons -- in the Solar System. It is not an active volcano. It has a canyon -- Valles Marineris -- that is as wide as the United States. It once had rivers, lakes and oceans of water. Scientists are trying to find out what happened to all this water and if there ever was (or still is!) life on Mars. It sometimes has dust storms that cover the entire planet.
    [Show full text]
  • Our Solar System
    Reader Moons of Our Solar System by Mick Roszel Genre Build Background Access Content Extend Language Expository • The Solar • Diagrams • Word Nonfi ction System • Captions Meanings • Planets and and Labels Moons • Glossary • Moon • Fact Box Geography Scott Foresman Reading Street 4.5.5 ì<(sk$m)=becbbi<ISBN 0-328-14211-5 +^-Ä-U-Ä-U 114211_CVR.indd4211_CVR.indd CCover1over1 33/8/05/8/05 99:26:20:26:20 PPMM Talk About It 1. What is a moon? 2. Look at the diagram on page 4. Describe three things itMoons shows about our of solar Oursystem. Write About It 3. How manySolar moons does S eachystem planet have? Make a graph on a separateby Micksheet Roszel of paper. Put one dot in the graph for each moon. 10 5 0 Mercury Venus Earth Mars Jupiter Extend Language A sphere is a round object, shaped like a ball or a planet. In sphere, pronounce the ph like f. Which of the following things can be called a sphere? the Earth’s moon a crater a soccer ball a coin Photographs Cover ©Omni-Photo Communications, Inc.; 1 ©Photo Researchers, Inc.; 2 ©Omni-Photo Communications, Inc.; 3 ©Bettmann/Corbis; 4 ©Luciano Corbella/DK Images; 5 (CR, BR) ©Corbis; 6 (CL) ©Photo Researchers, Inc., (BR) ©Tom Stack & Associates, Inc.; 7 ©Getty Images; 8 ©Digital Vision; 9 ©Jet Propulsion Laboratory/NASA; 10 ©Roger Ressmeyer/ NASA/Corbis. ISBN: 0-328-14211-5 Copyright © Pearson Education, Inc. All Rights Reserved. Printed in the United States of America. This publication is protected by Copyright, and permission should be obtained from the publisher prior to any prohibited reproduction, storage in a retrieval system, or transmission in any form by any means, electronic, mechanical, photocopying, recording, or likewise.
    [Show full text]
  • Family Guide to Mars - Field Test Version - © 2004 Space Science Institute
    For kids ages 6-12 and the adults they learn with! Contact: [email protected] Family Guide to Mars - Field Test Version - © 2004 Space Science Institute From the Development Team Dear Learning Enthusiast, The Guide's content develops and re-enforces four overall themes: • Comparing Earth and Mars as planets Welcome to the Family Guide to Mars! • The importance of water to life as we know it • The technology of Mars exploration This publication assumes little or no prior knowledge about • Seeing Mars in Earth’s sky Mars or astronomy in general. Feel free to jump around — the activities in this guide need We invite you to use the diverse activities and resources not be done sequentially. We encourage you to begin with here to have fun learning about Mars — The Red Planet! the Fill-in-the-Blanks Game on p. 22 to warm up your minds and hearts to Mars and its place in the Universe. The Guide includes an innovative collection of puzzles, pictures, poetry, and projects, all designed to stimulate Be sure to check out the FAQ at the back of the Guide, enjoyable co-learning experiences between kids aged which provides general background on Mars, with 6-12 and the caring adults in their lives. questions posed as kids tend to ask them. We crafted the “Gee Whiz Facts” to elicit the irresistible urge to tell someone Much learning in life takes place in informal environments else about them. Look for terms from the Glossary (on outside the classroom. We envision this Guide being of p.
    [Show full text]