Mercury Venus Mars
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1. A planetary magnetic field is created by metallic material in a planet's core and fluid motion within the core as the planet rapidly rotates. 2. A magnetic field protects a planet from having its atmosphere stripped away by solar winds. 3. Mercury has no atmosphere, a very weak magnetic field, temperatures that vary greatly between day and night, and an elliptical orbit.
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Mercury
Mercury is the smallest planet in the solar system and orbits the Sun every 88 Earth days. It rotates slowly, with a day lasting almost 60 Earth days. Mercury has almost no atmosphere and its surface is heavily cratered due to meteor impacts. It is named after the Roman messenger god Mercury and is the closest planet to the Sun, with surface temperatures varying greatly between very hot and very cold.
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Planet Mercury
Mercury is the closest planet to the sun and has thousands of huge craters from meteoroid and comet impacts. It rotates very slowly, resulting in a unusual sense of time. While astronomers previously believed Mercury's poles contained water ice, the MESSENGER spacecraft confirmed in 2011 there was no ice after sending back many pictures from its flybys of the planet.
Planet Saturn
Saturn is the sixth planet from the sun and named after the Roman god of agriculture. It is a gas giant with 18 known moons, the largest being Titan which is bigger than Mercury. Saturn's iconic rings are made of ice particles and span over 270,000 km wide, though they are only about 30 meters thick. The rings are composed of three main sections divided by darker gaps. Saturn orbits the sun every 29.5 years and spins rapidly on its axis, completing a day every 10 hours.
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Mercury is the closest planet to the sun and has thousands of huge craters from meteoroid and comet impacts. It rotates very slowly, resulting in a unusual sense of time. While astronomers previously believed Mercury's poles contained water ice, the MESSENGER spacecraft confirmed in 2011 there was no ice after sending back many pictures from its flybys of the planet.
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Saturn is the sixth planet from the sun and named after the Roman god of agriculture. It is a gas giant with 18 known moons, the largest being Titan which is bigger than Mercury. Saturn's iconic rings are made of ice particles and span over 270,000 km wide, though they are only about 30 meters thick. The rings are composed of three main sections divided by darker gaps. Saturn orbits the sun every 29.5 years and spins rapidly on its axis, completing a day every 10 hours.
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3. Mercury's surface temperature reaches a blistering 740 degrees kelvin during the day.
Venus presentation
Venus is named after the Roman god of beauty and was the second planet from the sun. It has an extremely hot surface temperature that would instantly kill any human visitors due to its dense carbon dioxide atmosphere and surface of lava and volcanoes. Despite being similar in size to Earth, Venus has extreme environmental conditions that are inhospitable to life as we know it compared to the more temperate climate on Earth.
Our solar system
The document provides information about the solar system including the eight planets and their characteristics. It describes the four inner planets - Mercury, Venus, Earth, and Mars which are made of rock and closest to the sun, and the four outer gas giants - Jupiter, Saturn, Uranus, and Neptune. It also discusses the planets' moons, Pluto's classification as a dwarf planet, and why some planets have more moons than others based on their gravitational pull and size.
Solar System Facts Slideshow
Solar System Facts - Free Printable Charts of Planets and Facts for Kids, Teachers, Parents - Ideal for School Project Ideas.
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Chapter 24 section 2 notes
Chapter 24
Section 2: The Inner Planets
Minersville Area School District
8th Grade General Science
Mr. Motuk
Chapter 24 section 2 notes
Chapter 24
Section 2: The Inner Planets
Minersville Area School District
8th Grade General Science
Mr. Motuk
Journey of Mangalyaan report
The document discusses India's Mars Orbiter Mission (MOM), which successfully placed an orbiter called Mangalyaan into orbit around Mars in 2014. It was India's first interplanetary mission. The key points are:
1) MOM's objectives included demonstrating India's technological capability to design, plan and manage an interplanetary mission as well as conducting scientific studies of Mars' surface, morphology, mineralogy and atmosphere.
2) The spacecraft carried five scientific payloads to analyze Mars' surface and atmosphere.
3) The mission achieved all its technological and scientific goals, making India the first nation to successfully reach Mars on its first attempt and the first Asian nation to reach Mars orbit.
Es Ch. 23 Solar System
The document provides an overview of our solar system, including:
1) It describes the major components of the solar system including the sun, eight planets, dwarf planet Pluto, asteroids, comets, and moons orbiting various planets.
2) Key details are provided about each of the inner and outer planets, such as their composition, atmospheric conditions, notable moons, and exploration by space probes.
3) The formation of the solar system from a large gas and dust cloud approximately 4.5 billion years ago is summarized based on the nebular hypothesis.
Planets
This document provides information about the planets in our solar system as well as asteroids, comets, and other celestial bodies. It details facts about each planet such as composition, size, atmospheric conditions, moons, and spacecraft missions. Key points include: the terrestrial planets like Earth are rocky, while the gas giants like Jupiter and Saturn have thick atmospheres composed primarily of hydrogen and helium; Venus' dense carbon dioxide atmosphere creates intense heat; Mars once had water and the potential for life; and asteroids and comets originate from the asteroid belt between Mars and Jupiter and the Kuiper Belt beyond Neptune's orbit. Spacecraft missions have revealed details of planets, moons, rings and other features of our solar system.
Mercury
Mercury is the planet closest to the Sun. It has a diameter of 4,878 km and rotates slowly, completing one rotation every 58.65 days. Mercury has a very thin atmosphere composed primarily of oxygen, sodium, potassium, and hydrogen. The MESSENGER spacecraft orbited Mercury from 2011-2015, obtaining high-resolution images and measurements of the planet's composition, geology, gravity field, magnetic field, and exosphere. MESSENGER's observations revealed that Mercury has an iron-rich core making up about 75% of the planet's radius and a complex geological history marked by volcanic activity and planetary contraction.
The planets
Mercury has many craters and cliffs from meteor impacts. It has extremes in temperature from 150°C to -180°C due to its proximity to the Sun and lack of atmosphere. Venus has a dense carbon dioxide atmosphere that causes intense greenhouse effect, making it the hottest planet with surface temperatures over 400°C. Mars has a thin atmosphere composed mostly of carbon dioxide, seasonal changes in color, and polar ice caps that grow and shrink with the seasons.
The planets
Mercury has many craters and cliffs from meteor impacts. It has extremes in temperature from 176°C to 427°C due to its proximity to the sun without an atmosphere. Venus has a dense carbon dioxide atmosphere that causes intense greenhouse effect, making it the hottest planet with surface temperatures over 462°C. Mars has polar ice caps and the largest volcano Olympus Mons, and its soil contains iron oxide that makes it appear red.
Chapter 23.2ppt
The document summarizes key facts about the terrestrial planets Mercury, Venus, and Mars. Mercury is the innermost planet with cratered highlands and long scarps cutting across its surface. It has extreme temperature variations from -173°C to 427°C. Venus is similar in size to Earth but is covered in dense clouds and has a surface temperature of 475°C due to a intense greenhouse effect. Mars has the largest volcanoes in the solar system and evidence that water may have flowed on its surface recently, though the atmosphere is only 1% as dense as Earth's and temperatures range from -70°C to -100°C.
1.Question DetailsMy NotesQuestion PartSubmissions Used(.docx
1.Question DetailsMy Notes
Question Part
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(Image Credit: NASA)
Select all that apply. Consider a generic Jovian planet with a cloud-top "surface" temperature of 85 K and an escape speed of 35 km/s. Assuming that the planet was not any hotter in the past, calculate if its atmosphere contains significant amounts of:
A. Hydrogen gas (H2)
B. Helium gas (He)
2.Question DetailsMy Notes
Question Part
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(Image Credit: NASA)
Select all that apply. Which of the following statements about the Galilean moons is true?
A. Because Io is closest to Jupiter, its tidal heating is the greatest, resulting in a mantle of molten rock and consequently in volcanic eruptions and lava flows that are hot enough to have evaporated the surface water, which was lost to space.
B. Because Europa is farther from Jupiter than Io, its tidal heating is less, resulting in a mantle of solid rock covered by an ocean of water.C. Because Ganymede is farther from Jupiter than Europa, its tidal heating is less, resulting in a mantle of solid rock covered by an ocean that probably consists of a slushy mix of water and ice.
D. Because Callisto is farther from Jupiter than Ganymede, its tidal heating is less, resulting in an interior that was never warm enough to differentiate: It remains an icy/rocky mix.
3.Question DetailsMy Notes
(Image Credit: NASA)
Divisions and gaps within Saturn's rings are caused by:
A. Orbital resonances with Saturn's moons
B. Small moons within the rings C. Shepherd moons
D. A & B
E. A & C
F. B & C
4.Question DetailsMy Notes
Question Part
Submissions Used
Select all that apply. In the following table, you will find the maximum surface temperature for each of the solar system's seven large moons. Generally speaking, the farther a moon is from the sun, the cooler it is:
Using these temperatures, calculate if ammonia (NH3) were to leak out of the interior onto the surface of each of these moons, which would be able to retain it as an atmosphere. (The molecular mass of ammonia is 17.)
A. Earth's moon
B. IoC. Europa
D. Ganymede
E. Callisto
F. Titan
G. Triton
5.Question DetailsMy Notes
Earth, Jupiter, Saturn, Uranus, and Neptune all have strong magnetic fields. To generate a magnetic field, a planet must have a layer that is both fluid, meaning it can move in complex ways, and conductive, meaning that electrons can flow through it easily. To generate a strong magnetic field, this layer, and hence the planet as a whole, must also rotate rapidly (which all of these planets do).
Which of the following materials is not responsible for generating any of these planets' magnetic fields?
A. Liquid iron
B. Metallic hydrogen C. Molecular hydrogen
D. Water-ammonia slush
6.Question DetailsMy Notes
Which of the following planets does not have a significant internal source of heat?
A. Jupiter
B. Saturn C. Uranus
D. Neptune
7.Question DetailsMy Notes
Question Part
Submissions Used
(Image Credit: Gemini Observatory/Lyn.
Dtu10e lecture ppt_ch07
The document discusses features of the planet Mercury such as its heavily cratered surface, dormant volcanoes, and substantial iron core. It also describes Venus' thick, poisonous atmosphere and rolling hills with few impact craters. Finally, it mentions that Mars was once thought to have canals but was found to have water on its surface in the past and may still have underground water reserves today. It provides images and details about the geological features and climates of these three planets.
Op ch02 lecture_earth3
The earliest material found in the Solar System is dated to 4.5672±0.0006 by] therefore, it is inferred that the Earth must have been formed by accretion around this time. By 4.54±0.04 by the primordial Earth had formed. The formation and evolution of the Solar System bodies occurred in tandem with the Sun. In theory a solar nebula partitions a volume out of a molecular cloud by gravitational collapse, which begins to spin and flatten into a circumstellar disk, and then the planets
grow out of that in tandem with the star. A nebula contains gas, ice grains and dust
Origins of our solar system
The document provides information about the origins of the solar system, including details about the Sun, Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, Neptune, and a prediction about the future of the solar system. It describes characteristics of each planet such as their composition, size, distance from the Sun, moons, and exploration by spacecraft.
Mars Planet
Mars is approximately half the size of Earth and has a thin atmosphere composed primarily of carbon dioxide. It has the largest volcano and canyon in the solar system. Early concepts suggested canals and life on Mars but spacecraft like Mariner 4 revealed only impact craters and naturally occurring channels. Viking landers found no clear evidence of living microbes. However, past rover missions like Spirit, Opportunity, and Curiosity continue to find evidence that water once flowed on the Martian surface, making the possibility of past life an ongoing area of investigation. Future exploration plans aim to further understand Mars' potential for habitability.
Ch09 inner planets
The four terrestrial planets - Mercury, Venus, Earth, and Mars - are similar in size and structure. They orbit in the inner solar system and are too small to retain thick hydrogen atmospheres. Mercury is the smallest and hottest planet, with extensive volcanic plains and impact craters. Venus has a dense, toxic atmosphere that causes a strong greenhouse effect and maintains surface temperatures over 400°C. Mars has the largest volcano in the solar system, Olympus Mons, and polar ice caps that vary in size with the seasons.
Space Lecture
This document provides a summary of key topics in space exploration including:
1) Early space probes and manned missions that explored space starting in the 1950s and 1960s including Sputnik 1, Vostok 1, Mercury, and Apollo missions.
2) Components of rockets such as the launch vehicle, control module, service module, and lunar module.
3) Properties of the inner planets Mercury, Venus, Earth, and Mars including their atmospheres, temperatures, moons, and geological features.
4) Formation and characteristics of the moon including its dark surface, lack of erosion, and differences between the highlands and maria regions.
New solar system presentation
The document summarizes the formation of the solar system based on the nebular hypothesis. It explains that the solar system formed from the gravitational collapse of a giant gas and dust cloud about 4.6 billion years ago. As the cloud collapsed and spun faster, the heavier elements collected in the center to form the inner terrestrial planets, while the outer parts formed the outer gaseous jovian planets. Over time, small particles collided and merged to form larger bodies called planetesimals, which eventually formed the planets.
Solar system
The document provides information about the components of our solar system, including the sun, terrestrial planets, asteroid belt, jovian planets, Kuiper belt, and Oort cloud. It describes each of the terrestrial planets (Mercury, Venus, Earth, Mars) as well as their characteristics such as composition, density, atmosphere, size, moons, rotation, and temperature. It also describes the gas giant planets Jupiter and Saturn and ice giants Uranus and Neptune, including their moons. The sun is identified as being at the center of the solar system and providing energy for life on Earth through photosynthesis.
Touring our solar system (astronomy)
The document summarizes how the planets in our solar system formed and their key characteristics. It explains that the solar system originated from a large cloud of dust and gas that contracted under gravity, with most matter forming the Sun and the remainder forming a disk from which the planets accreted. The inner, terrestrial planets like Mercury, Venus, Earth and Mars are rocky, while the outer, Jovian planets like Jupiter, Saturn, Uranus and Neptune are gas giants due to forming farther from the Sun where ices could condense. The document contrasts attributes of the inner and outer planets such as size, density, chemical makeup and atmospheres.
Astronomy - State of the Art - Planets
Astronomy - State of the Art is a course covering the hottest topics in astronomy. In this section, the Solar System is explored, including place where biology might exist.
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1.Question DetailsMy NotesQuestion PartSubmissions Used(.docx
1.Question DetailsMy NotesQuestion PartSubmissions Used(.docx
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Mercury Venus Mars
- 1. What creates a planetary magnetic field? 1. Metallic material in the core 2. (a) Fluid Motion of the core OR (b) Rapidly Rotating planet
- 2. What benefit is a magnetic field? - Protects the planet from atmosphere stripping solar winds.
- 3. Mercury -Roman god of Travel
- 4. Mercury - Basic Information No Atmosphere Very Weak Magnetic Field (1% of Earth’s) Rotates 3 times for every 2 revolutions Temperature variations: Shadow: -300F Sunlight: 800F Highly Elliptical Orbit 29 million miles to 43 million miles
- 5. Mercury Transit The planet passes in front of the Sun.
- 6. ME-S-S-EN-GE-R Mercury Surface Space Environment Geochemistry and Ranging
- 7. Text
- 8. Water Ice -Found in Permanent Shadows of craters.
- 9. Venus Roman god of Love
- 10. Venus - Basic Information Revolves once every 243 Earth Days Rotates once every 224 Earth Days Thick CO2 atmosphere (100 times thicker than Earth’s) Surface Temperature = 900F
- 11. Venus - Basic Information Runaway Greenhouse Effect No moons No magnetic field No plate tectonics
- 12. Venera Spacecraft Russian - First landing on another planet.
- 13. Text
- 14. Mars Roman god of War
- 15. Mars Half the size of the Earth
- 16. Mars - basic info Atmosphere 1% as thick as Earth Mostly CO2 Temperatures can range from -200 F up to 70 F No magnetic field
- 17. Mars Exploration -1970’s: Viking Landers -1980’s: Numerous failed missions -1996: Pathfinder Rover -2004: Mars Exploration Rovers (Spirit & Opportunity) -2008: Mars Phoenix Lander -2012: Mars Science Laboratory (Curiosity)
- 18. Anatomy of a Mars Landing Compare three different approaches
- 19. Text Water in Mars’ past? CONFIRMED
- 21. Mars Subsurface salty water may still exist on Mars
- 23. Mars has 2 small moons: