Mercury Mythology - Hermes – The messenger god) 1 st ever color photo of Mercury by MESSENGER probe; 2008.

Slides:



Advertisements
Similar presentations
The Solar System Chapter 12 Section 1 Pgs
Advertisements

 The Sun  4 Inner planets  4 Jovian planets  8 Dwarf planets  30 objects highly likely to be dwarf planets  60 objects which are likely to be dwarf.
The Solar System and its Planets. The milky way (seen from Bryce Canyon, UT)
Mercury Venus Earth Mars Jupiter Saturn Uranus Neptune Dwarf Planets Sun Eris Pluto Ceres By Michelle Stephens.
The Solar System By: Seemani Dash.
The Planets. Mercury The Messenger God 0 Closest planet to the Sun AU 0 Main gases: Na, O, He -300 °F at night 800 °F during the day No moons 0.
Venus is the second planet from the Sun and is the second brightest object in the night sky after the Moon. Venus is the second largest terrestrial planet,
Jaye R. Cashen Basic Facts about Venus Venus is named after the roman goddess of love and beauty Located between Earth and Mercury Covered with thick.
Mercury, seen from Earth through a moderate telescope.
Venus Astronomy 311 Professor Lee Carkner Lecture 11.
Venus Astronomy 311 Professor Lee Carkner Lecture 11.
Interiors of Terrestrial Planets. Mercury MEAN RADIUS: km MASS: (Earth=1) DENSITY: 5.43 (g/cm^3) GRAVITY: (Earth=1) ORBIT PERIOD:
Mercury Astronomy 311 Professor Lee Carkner Lecture 10.
Astronomy 1 – Winter 2011 Lecture 17; February
The Terrestrial Planets Astronomy 311 Professor Lee Carkner Lecture 9.
Astronomy Picture of the Day. Mercury Mass = M Earth Radius = 0.38 R Earth  Surface Temp: K Average distance from Sun =.39 AU Moonlike:
Venus Astronomy 311 Professor Lee Carkner Lecture 11.
Comparative Planetology
Terrestrial Planets- Mercury & Venus THE SOLAR SYSTEM.
Our Solar System An introduction to our planets.
Venus The bright and morning (evening) star. Moon & Venus Morning of April 22, 2009
Chapter 16 Section 3 Inner Planets.
Formation of the Solar System Chapter 27 page 684-
Unit 13 Planets. What is a planet? Old Definition A planet is a body that orbits a star, shines by reflecting the star's light and is larger than an.
The Sun Earth Science - Mr. Gallagher. The Sun is the Earth's nearest star. Similar to most typical stars, it is a large ball of hot electrically charged.
The Terrestrial Planets, Part I
Atmospheres of the Planets By Danielle Stroup. Introduction-Definitions Atmosphere consists of molecules and atoms moving at various speeds Temperature.
Sin’Kira Khan & Dane Fujinaka
Crash Landing Activity First, get into teams of three to five (I will assign) and create a list of items you would need to bring to survive an extended.
Our Solar System 6 th grade Earth’s movement is constant! Earth’s orbit – Sun is at the center – Orbit: movement of an object around another.
Venus is named after the Roman goddess of love and beauty. Venus rotates on it’s axis every 243 earth days. Venus’ mean radius is 3,760.
Solar System Inner planets Outer planets.
Big Bang theory Parts of our solar system Planet characteristics Galaxies Constellations Nebulas.
(Terrestrial) Planetary Atmospheres II.  Atmospheres consist of exospheres only  Take either of their atmospheres, could “almost store them in a dorm.
Our Solar system YouTube - The Known Universe by AMNH.
A yellow star made of HYDROGEN AND HELIUM GAS. The sun gives off ENERGY!
The Solar System By Megan Zelenka and Sophia Yearoo.
MERCURY Q: Why are there so many craters?. Mercury.
1 Inner or Terrestrial Planets All the inner planets formed at the same time. Their composition is also very similar. They lack the huge atmospheres of.
28 Sep 2000ASTR103, GMU, Dr. Correll1 Ch 06--Other Terrestrial Planets.
Venus By: Shahrukh and Michael. Geological Features ► We find evidence for many of the same geological features found on Earth: canyons, volcanoes, lava.
The Inner Planets 20.3.
Zackery Harris, Daniel Buennostro, Chris Hiltzman.
The Sun 99.8% of the mass of the solar system is in the Sun.
Earth and Space Our Solar System Our solar system is made up of: Sun Eight planets Their moons Asteroids Comets Meteoroids.
Full name Period III. Chapter 14, section 3: The Inner Planets A. The inner planets: are the four terrestrial planets that are closest to the sun. Mercury.
The Solar System (On the next page, click on a planet to learn about it, then click on the spaceship to go back to the Solar System)
The Solar System. Solar System the sun and all things orbiting around it, including the eight major planets, their satellites, and all the smaller pieces.
Our Earth & Moon (Chapter 16). Student Learning Objectives Compare and contrast interior structures of the Earth & Moon Describe surface features for.
VENUS. “Twin” or “Sister” planet of the earth  similar size, mass, density; interior should also be similar with iron core, mantle, crust But totally.
The Solar System Inner and Outer Planets
Know about the Sun’s Energy Know about the Sun’s Core, Atmosphere, and Sunspots Comprehend the Solar System’s Structure The Sun and It’s Domain.
Earth and the Other Terrestrial Worlds
Size: km (0.949 Earths)‏ Orbit: 108,208,930 km (0.723 AU)‏
INNER PLANETS Terrestrial Planets are the Four planets closest to the sun. These planets have rocky terrain, and have higher temperatures due to receiving.
Chapter 29 The Solar System
The Solar System: Inner Planets
EXPLAIN THE NEBULAR HYPOTHESIS OF THE ORIGIN OF THE SOLAR SYSTEM. DESCRIBE HOW THE PLANETS FORMED DESCRIBE THE FORMATION OF THE LAND, THE ATMOSPHERE, AND.
What are the Inner planets?
The Solar System.
Copyright © 2010 Pearson Education, Inc. The Terrestrial Planets.
The Solar SystemSection 2 The Inner Planets 〉 How are the inner planets similar to one another? 〉 The terrestrial planets are relatively small and have.
Mercury By Jayda, Baya,lucas. How Did Mercury Get It’s Name? In astronomy mythology, Mercury was the Roman version of the Greek god Hermes. He was the.
Planets Ch. 21 Notes.
The Inner Planets.
Mercury Venus Earth Mars
Venus Second planet from the Sun
Chapter 23 The Solar System
The Solar System.
Presentation transcript:

Mercury Mythology - Hermes – The messenger god) 1 st ever color photo of Mercury by MESSENGER probe; 2008

Mercury Transit across Sun 1 st ever color photo of Mercury by MESSENGER probe; 2008

Mercury Mapped by Mariner 10

Mercury vs. Earth & Moon 1/6 size of Earth

Mercury Images by Mariner 10

Mercury Statistics: *.4 A.U. From Sun * 1/3 Size of Earth * Orbital Period = 3 Months *Rotation Period = 88 Days * Surface Gravity = 1/6 of Earths * The planet is too small to hold an atmosphere

Atmosphere: There is no atmosphere heat is not trapped on the planet. it is VERY HOT during the day, and VERY COLD during the night Mercury is NOT the hottest or coldest planet.

core 1.Very Large 2.Solid 3.Iron Mercury has a disproportionately large Iron core. It should be cooled and solid. However, MESSENGER flyby data indicates the core is partially molten. This contradicts current theories.

Lobate scarps Definition – curved cliffs Cause = When the core cooled,it shrunk, causing the crust to collapse.

Mercury Missions to Mercury Mariner 10 Launched Nov 1973 Flyby March 1974 MESSENGER Launched Aug 2004 Orbit insertion March 2011

Mercury MESSENGER Orbit Insertion –> Launch – E – V – V - M – M - M

Mercury MESSENGER Orbit Insertion –> Launch – E – V – V - M – M - M

Venus Aphrodite – The goddess of Love The Morning/Evening Star/Sister Planet

Venus Statistics Distance -.73 A.U. From Sun Size – Same Diameter as Earth

More Statistics Orbital Period –.6 Years Rotation Period – 243 days Surface Gravity –.9 of Earths

Venus Atmosphere Runaway Greenhouse Effect –Visible light from sun hits the surface –Surface reradiates the energy in the form of infrared –Clouds block some of the IR from escaping –Surface gets hotter

Runaway Greenhouse Effect Results CO 2 Atmosphere NO WATER!

CO 2 Atmosphere

No Water!

Atmospheric Conditions 1.Pressure 90x that of Earths 2. Very dry, no surface water 3. Sulfuric Acid in Clouds Atmosphere 4. Temperature 900 F 5. Wind Speed up to 250 Miles per Hour.

Venus Weather Images/Video from Venus Express Orbiter Twin cyclones: two storms with low- pressure centers that causes a circular pattern of winds to form.

Weather Vortex Storms: –huge swirling vortex of clouds around Venus' southern pole. –changes shape within just a few days –The rotation of Venus deflects them sideways so they swirl together, like water going down the drain of a bathtub.rotation of Venus

(vortex)

Venus Solar Storms i.Venus does not have a magnetic field. ii. Solar Wind erodes away the atmosphere.

Venus Missions Venera 9-14 – – Landers ( First & only images of Surface )

Venus Surface Images from Venera 13 probe

Venus Missions Magellan – 1989 – Orbiter – Created Radar Map of Surface

Venus Missions Magellan – Radar Map ~8 min magellan_mapping_venus.wmv

Venus Missions Magellan – Radar Map

Venus Missions Pioneer Venus 1 & – Orbiters & Descent Probes

Venus Missions Venus Express – 2005 to present – Orbiter Animation of Venus Express Studying Venus

Venus Missions Venus Express ~5 min

Venus Although Venus is often called Earth’s Twin or Sister planet. The only similarities is the size. Almost every other feature makes Venus very different from Earth.

Earth MESSENGER animation Leaving earth.

Earth

Atmosphere -78% nitrogen, 21% oxygen Distance -1 au from sun (93,000,000 miles) Contains water in all 3 phases Surface Gravity – 9.8 m/s Rotation – 1 day Orbit – 1 year

Earth Greenhouse Effect -Has Liquid Water (Some Water Vapor in Atmosphere) -Water vapor keeps planet warm ( main greenhouse gas ) -Ozone Layer prevents water from Disassociating

Earth Greenhouse Icehouse Technically, Earth is currently undergoing an Icehouse effect. however, most of the time, Earth is in a Greenhouse effect.

Earth Icehouse effect : - Anytime there is a continent over any of the poles, the resulting ice sheet reflects large amounts of Solar Radiation into space -causing the Earth to cool down. Image from NASA Earth Observatory

Earth Greenhouse Icehouse Technically, Earth is currently undergoing an Icehouse effect. however, most of the time, Earth is in a Greenhouse effect. GondwanalandPangaeaAntarctica

Earth Icehouse effect As long as Antarctica is at the South Pole, the Earth will continually be thrown into Glaciation periods. We are currently at the end of an Interglacial period.

Earth 70 Atmospheres of CO2 is trapped in Earths Rocks. If all of this CO2 were released, which planet would we look like? Only place we know of that supports life - 4 reasons: 1.Correct distance from sun 2.Natural/Stable greenhouse effect 3.Ozone Layer & Magnetic Field 4.Presence of Liquid Water

Planet Guidelines The IAU therefore resolves that planets and other bodies in our Solar System be defined into three distinct categories in the following way: (1) A planet 1 is a celestial body that (a) is in orbit around the Sun, (b) has sufficient mass for its self- gravity to overcome rigid body forces so that it assumes a hydrostatic equilibrium (nearly round) shape, and (c) has cleared the neighbourhood around its orbit. (2) A dwarf planet is a celestial body that (a) is in orbit around the Sun, (b) has sufficient mass for its self-gravity to overcome rigid body forces so that it assumes a hydrostatic equilibrium (nearly round) shape 2, (c) has not cleared the neighbourhood around its orbit, and (d) is not a satellite. (3) All other objects 3 orbiting the Sun shall be referred to collectively as "Small Solar System Bodies".

Planet Guidelines (1) A planet is a celestial body that –(a) is in orbit around the Sun, –(b) has sufficient mass for its self-gravity to overcome rigid body forces so that it assumes a hydrostatic equilibrium (nearly round) shape, and –(c) has cleared the neighbourhood around its orbit.

Planet Guidelines (2) A dwarf planet is a celestial body that –(a) is in orbit around the Sun, –(b) has sufficient mass for its self-gravity to overcome rigid body forces so that it assumes a hydrostatic equilibrium (nearly round) shape 2, ( –c) has not cleared the neighbourhood around its orbit, and –(d) is not a satellite.

Planet Guidelines (3) All other objects 3 orbiting the Sun shall be referred to collectively as "Small Solar System Bodies".

Video Links Earth from Spaceshuttle – &feature=relatedhttp:// &feature=related Qhttp:// Q &feature=PlayList&p=0D959158C1FC558F&pla ynext=1&index=21http:// &feature=PlayList&p=0D959158C1FC558F&pla ynext=1&index=21

Mars Go to inner_mars.ppt