Solar System 3 Part Cards

Total Page:16

File Type:pdf, Size:1020Kb

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. Earth is the only planet which has life Jupiter spins very fast which makes it Scientists think there may have been on it. looked striped from the clouds being flowing rivers on Mars long ago but pulled into bands. The Earth is tilted. When your part of they’re gone now. the Earth is tilted toward the sun, it’s Jupiter is a big ball of gas and does not Scientists have sent up robots called summer. When it’s tilted away from the have a solid surface. rovers to roll across Mars taking pic- sun it’s winter. Jupiter has at least 63 moons. Four tures and studying the planet. Earth spins counter-clockwise. are called Europa, Callisto, Io and Ganymede. Saturn Uranus Neptune Moon Ceres Pluto Neptune is the farthest planet from the Uranus is tipped onto its side. Saturn has thousands of rings. The sun out of the big planets. Scientists think that a huge space ob- rings are made up of billions of bits of Neptune is made up of gas. ject hit it long ago. icy rocks. Some bits are as tiny as dust and others are as big as mountains. Winds on Neptune blow more than a Uranus spins in the opposite direction thousand miles an hour. to Earth. Saturn is a gas planet with no solid surface. It takes Neptune 165 years to travel Uranus is the coldest of the eight big around the sun. planets. Saturn has at least 53 moons. Saturn’s Uranus has 13 rings. biggest moon is called Titan. 4 other Neptune has a big storm called the moons are Rhea, Iapetus, Dione and Great Dark Spot. Uranus has at least 27 moons. One is Tethys. Neptune has at least 13 moons. Triton named Miranda. is Neptune’s largest moon. Proteus is Uranus is a gas planet. the second largest and Nereid the third largest. Pluto is a dwarf planet. It is in the Ceres is a dwarf planet. The moon travels around Earth. It Kuiper Belt. takes about 27 days for the moon to go Pluto used to be considered a regular around the Earth. planet but scientists now call it a dwarf The moon is actually dark, it looks planet. bright because the sun reflects off it’s Pluto spins clockwise. surface. The shape of the moon that we see Pluto has a moon called Charon. from Earth changes because the Earth casts a shadow on it. The same side of the moon always faces earth. Astronauts landed on the moon 6 times. Haumea Makemake Eris Phobos Deimos Europa Eris is the largest of the dwarf planets. Makemake is a dwarf planet. Haumea is a dwarf planet. It takes Makemake 310 years to travel Haumea is an unusual shape. around the sun. Scientists think something smashed into Haumea long ago. This may have created Haumea’s two moons, Namaka and Hi’iaka. Europa is one of Jupiter’s moons. Deimos is one of Mars’s moons. It is Phobos is one Mars’s moons. It is very Europa may have deep, ice-covered very close to Mars. close to Mars. oceans. Deimos has a funny shape, like a Phobos has a funny shape, like a potato. potato. Callisto Io Ganymede Titan Rhea Iapetus Ganymede is one of Jupiter’s moons. Io is one of Jupiter’s moons. Callisto is one of Jupiter’s moons. It is the biggest moon in our solar Io is covered by volcanoes. Callisto is about the same size as system. Mercury. Iapetus is one of Saturn’s moons. Rhea is one of Saturn’s moons. Titan is Saturn’s biggest moon. Titan is bigger than Mercury. Dione Tethys Miranda Triton Proteus Nereid Miranda is one of Uranus’s moons. Tethys is one of Saturn’s moons Dione is one of Saturn’s moons. Miranda has canyons 12 times deeper than the Grand Canyon on Earth. Nereid is Neptune’s third largest moon. Proteus is Neptune’s second largest Triton is Neptune’s largest moon. moon. Triton is one of the coldest places in our solar system. Triton has volcanos that burst and freeze instantly. The gas and dust falls back to the surface like snow. Charon Vesta Asteroid Ida Asteroid comet spiral galaxy stars Ida is an asteroid. Asteroids are made Vesta is an asteroid. Asteroids are Charon is Pluto’s moon. up of leftover bits and pieces of rock made up of leftover bits and pieces of The same side of Charon always faces and metal in space that did not rock and metal in space that did not Pluto. become planets or moons. become planets or moons. Charon is about half as big as Pluto. There are millions of asteroids in our There are millions of asteroids in our solar system. Many are in the asteroid solar system. Many are in the asteroid belt. belt. Asteroids orbit the sun. Asteroids orbit the sun. Ida has it’s own moon called Dactyl. On a clear night you can see 3,000 A galaxy is a group of stars, gas and A comet is made up of icy gas and stars with your eyes. But there are dust held together by gravity. rock. billions more that you cannot see. Spiral galaxies are the shape of a When a comet gets too close to the sun Stars are made up of hot gases. pinwheel. it begins to melt which forms a tail The hottest stars shine blue, the We live in a Spiral galaxy. behind it. The tail can stretch for coolest stars shine red. millions of miles. After the sun, the closest star to Earth There are billions of comets in the is Proxima-Centauri. Light from this Kuiper Belt. star takes 4 years to reach Earth. irregular galaxy Helix Nebula Bug Nebula meteoroids Pillars of Creation elliptical galaxy When some stars die they explode. A When some stars die they explode. A A galaxy is a group of stars, gas and nebula is the leftover start dust after nebula is the leftover start dust after dust held together by gravity. this explosion. this explosion. An Irregular galaxy does not have a New stars are born inside the nebula. New stars are born inside the nebula. particular shape. Gas and dust pull together and create Gas and dust pull together and create young stars. young stars. The Bug Nebula looks like a butterfly. The Helix Nebula looks like an eye. A galaxy is a group of stars, gas and When some stars die they explode. A A meteoroid is a small piece of rock or dust held together by gravity. nebula is the leftover start dust after metal flying through space. It is much An elliptical galaxy is the shape of an this explosion. smaller than an asteroid. ellipse. New stars are born inside the nebula. When a meteoroid enters Earth’s Gas and dust pull together and create atmosphere it begins to burn and glow, young stars. looking like a streak or shooting star. Pillars of Creation is part of the Eagle Most burn up before they hit earth but Nebula. some don’t. If they survive and hit earth they are called meteorites. .
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]
  • 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]
  • 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]
  • Flags and Footprints on Phobos and Deimos
    Flags and Footprints on Phobos and Deimos By Daniel A. O’Neil Abstract Scanners on balloons and rovers digitize the Mars surface. Remote controlled rockets launch sample containers. A Robonaut 5 captures the containers. A flight engineer uploads the surface models to a virtual reality metaverse for the public. Robonaut 5 assists with excursions to Phobos and Deimos. Prologue Sept. 13, 2030 A Block-2 Space Launch System (SLS), with a capacity of 130 MT, launches a Solar Electric Propulsion (SEP) Mars Transfer Vehicle (MTV); the USS Minerva starts her 900 day voyage to Mars. Oct. 18, 2030 A Block-2 SLS launches a SEP MTV named Minerva’s Owl. Hauling a stage containing Liquid Oxygen (LOX) and methane tanks, Minerva’s Owl flies to Mars. July 28, 2032 A Block-2 SLS launches an Exploration Upper Stage (EUS) with LOX and methane tanks, a propulsion system, and a truss with robotic arms. Aug. 4, 2032 A Block-2 SLS launches an upper stage with liquid oxygen and methane tanks. An Orbital Maneuvering Vehicle (OMV) moves the stage into a position where the robotic arms on the EUS truss can pull the tank stage and lock the stage to the truss. Aug. 11, 2032 A Block-2 SLS launches another tank stage and an OMV moves the stage to a position where the EUS robotic arms attach the stage to the truss. Aug. 19, 2032 A Block-2 SLS launches a Bigelow Aerospace Olympus habitat. (BA 2100) Aug. 24, 2032 A Block-2 SLS launches an upper-stage with an Orion spacecraft, solar power system, and an OMV.
    [Show full text]
  • Exploration Leading to Low-Latency Telepresence on Mars from Deimos
    Exploration Leading to Low-Latency Telepresence on Mars from Deimos Daniel R. Adamo 503-585-0025 Independent Astrodynamics Consultant [email protected] Paul A. Abell, NASA-Johnson Space Center Robert C. Anderson, Jet Propulsion Laboratory/California Institute of Technology Brent W. Barbee, NASA-Goddard Space Flight Center Joshua B. Hopkins, Lockheed Martin Thomas D. Jones, Senior Research Scientist, Institute for Human and Machine Cognition Robert R. Landis, NASA-Johnson Space Center James S. Logan, Space Enterprise Institute Daniel D. Mazanek, NASA Langley Research Center Gregg Podnar, Robot Systems Architect, Aeolus Robotics Exploration Leading to Low-Latency Telepresence on Mars from Deimos 1 Introduction The strategy of using robotic precursor spacecraft to prepare for human space exploration at a common venue has its roots in the Lunar Orbiter [1] and Surveyor [2] missions leading to initial Apollo Program human landings on the Moon in 1969. In connection with the current Artemis Program's human return to the Moon, robotic precursors are being instigated through NASA's Commercial Lunar Payload Services (CLPS) initiative [3]. These lunar precursors tend to be science-centered, but they also incorporate technology demonstration objectives addressing human factors and in-situ resource utilization (ISRU) knowledge gaps. Looking farther along NASA's human exploration roadmap into the 2030s and beyond, venues proximal to Mars become prominent. Robotic precursors in this context begin with the first flyby spacecraft Mariner 4 in 1965 [4], the first orbiter Mariner 9 in 1971 [5], the first lander Viking 1 in 1976 [6], and the first rover Sojourner in 1997 [7]. Exploration with these precursors and their successors has been impeded by enormously high data latency compared with lunar communications.
    [Show full text]
  • Martian Moon's Orbit Hints at an Ancient Ring of Mars
    Martian Moon’s Orbit Hints at an Ancient Ring of Mars PRESS RELEASE DATE June 2, 2020 CONTACT Rebecca McDonald Director of Communications SETI Institute [email protected] +1 650-960-4526 Photo credit: https://solarsystem.nasa.gov/moons/mars-moons/deimos/in-depth/ June 2, 2020, Mountain View, CA – Scientists from the SETI Institute and Purdue University have found that the only way to produce Deimos’s unusually tilted orbit is for Mars to have had a ring billions of years ago. While some of the more massive planets in our solar system have giant rings and numerous big moons, Mars only has two small, misshapen moons, Phobos and Deimos. Although these moons are small, their peculiar orbits hide important secrets about their past. For a long time, scientists believed that Mars’s two moons, discovered in 1877, were captured asteroids. However, since their orbits are almost in the same plane as Mars’s equator, that the moons must have formed at the same time as Mars. But the orbit of the smaller, more distant moon Deimos is tilted by two degrees. “The fact that Deimos’s orbit is not exactly in plane with Mars’s equator was considered unimportant, and nobody cared to try to explain it,” says lead author Matija Ćuk, a research scientist at the SETI Institute. “But once we had a big new idea and we looked at it with new eyes, Deimos’s orbital tilt revealed its big secret.” This significant new idea was put forward in 2017 byĆ uk’s co-author David Minton, professor at Purdue University and his then-graduate student Andrew Hesselbrock.
    [Show full text]
  • The Formation of the Martian Moons Rosenblatt P., Hyodo R
    The Final Manuscript to Oxford Science Encyclopedia: The formation of the Martian moons Rosenblatt P., Hyodo R., Pignatale F., Trinh A., Charnoz S., Dunseath K.M., Dunseath-Terao M., & Genda H. Summary Almost all the planets of our solar system have moons. Each planetary system has however unique characteristics. The Martian system has not one single big moon like the Earth, not tens of moons of various sizes like for the giant planets, but two small moons: Phobos and Deimos. How did form such a system? This question is still being investigated on the basis of the Earth-based and space-borne observations of the Martian moons and of the more modern theories proposed to account for the formation of other moon systems. The most recent scenario of formation of the Martian moons relies on a giant impact occurring at early Mars history and having also formed the so-called hemispheric crustal dichotomy. This scenario accounts for the current orbits of both moons unlike the scenario of capture of small size asteroids. It also predicts a composition of disk material as a mixture of Mars and impactor materials that is in agreement with remote sensing observations of both moon surfaces, which suggests a composition different from Mars. The composition of the Martian moons is however unclear, given the ambiguity on the interpretation of the remote sensing observations. The study of the formation of the Martian moon system has improved our understanding of moon formation of terrestrial planets: The giant collision scenario can have various outcomes and not only a big moon as for the Earth.
    [Show full text]
  • Moon-Miners-Manifesto-Mars.Pdf
    http://www.moonsociety.org/mars/ Let’s make the right choice - Mars and the Moon! Advantages of a low profile for shielding Mars looks like Arizona but feels like Antarctica Rover Opportunity at edge of Endeavor Crater Designing railroads and trains for Mars Designing planes that can fly in Mars’ thin air Breeding plants to be “Mars-hardy” Outposts between dunes, pulling sand over them These are just a few of the Mars-related topics covered in the past 25+ years. Read on for much more! Why Mars? The lunar and Martian frontiers will thrive much better as trading partners than either could on it own. Mars has little to trade to Earth, but a lot it can trade with the Moon. Both can/will thrive together! CHRONOLOGICAL INDEX MMM THEMES: MARS MMM #6 - "M" is for Missing Volatiles: Methane and 'Mmonia; Mars, PHOBOS, Deimos; Mars as I see it; MMM #16 Frontiers Have Rough Edges MMM #18 Importance of the M.U.S.-c.l.e.Plan for the Opening of Mars; Pavonis Mons MMM #19 Seizing the Reins of the Mars Bandwagon; Mars: Option to Stay; Mars Calendar MMM #30 NIMF: Nuclear rocket using Indigenous Martian Fuel; Wanted: Split personality types for Mars Expedition; Mars Calendar Postscript; Are there Meteor Showers on Mars? MMM #41 Imagineering Mars Rovers; Rethink Mars Sample Return; Lunar Development & Mars; Temptations to Eco-carelessness; The Romantic Touch of Old Barsoom MMM #42 Igloos: Atmosphere-derived shielding for lo-rem Martian Shelters MMM #54 Mars of Lore vs. Mars of Yore; vendors wanted for wheeled and walking Mars Rovers; Transforming Mars; Xities
    [Show full text]
  • Tuesday 6Th June 2017: "Fear and Dread" - John Rosenfield (HAS)
    Tuesday 6th June 2017: "Fear and Dread" - John Rosenfield (HAS) John’s main purpose was to invite us on a journey to the planet Mars without fear or dread. Viking images of Mars show ice caps, dark patches and a red surface, which is due to iron in the rocks. However, over the years the red planet, accompanied by its moons Phobos and Deimos (meaning fear and dread), has symbolised war with the mythological god Mars/Ares, noted for being aggressive and courageous – ready to fght any batle. Patrick Moore had this to say in his writngs about Mars and its ‘canals’: “Lowell was convinced that the Red Planet supported an advanced technical civilisaton, and that the canals represented an irrigaton system to carry water from the polar snows to the deserts of the equator. Lowell’s views met with considerable oppositon even in his own lifetme, though he remained unshaken up to the tme of his death in 1916. The idea of intelligent Martans was regarded as distnctly dubious. On the other hand the idea that the dark areas were due to vegetaton met with strong support, and up to 1965 very few astronomers doubted it”. Phobos and Deimos are tny moons at 27 km and 12.5 km respectvely. (1). (1) To put this into perspectve, New Horizons is currently on its way to visit a Kuiper Belt object just 40 km across, which although very small is nevertheless larger than Mars’ moons. Phobos orbits just 6000 km above the planet’s surface and is slowly spiraling inwards where at some point in the future it will break up, forming a ring around Mars before some of the bits crash into the surface.
    [Show full text]