Chapter 27.3 The Inner Planets

Slides:



Advertisements
Similar presentations
Ch. 29 Sec. 2 Terrestial Planets. First four  Mercury, Venus, Earth, Mars  Solid, Rocky surfaces.
Advertisements

The Inner Planets Lesson 4.
Clicker Questions Chapter 6 The Terrestrial Planets Copyright © 2010 Pearson Education, Inc.
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,
The Inner Planets  The inner planets are the 4 planets closest to the sun:  Mercury  Venus  Earth  Mars  The four inner planets are small and dense.
The inner planets What do the inner planets have in common? what are their characteristics?
The Inner Rocky Planets By:Joyce Lee and Kay LimAnd Kay Lim.
THE INNER PLANETS.
Chapter 16 Section 3 Inner Planets.
The Solar System.
Chapter 21 Sections 1-3 Review PowerPoint. Know the order in which the planets orbit the Sun: Mercury Venus Earth Mars Jupiter Saturn Uranus Neptune.
Chapter 27 The Solar System.
A Tour through the Solar System. The Inner Planets Include Mercury, Venus, Earth, and Mars Include Mercury, Venus, Earth, and Mars Also known as terrestrial.
Astronomy 1. Weekly Quiz  In place of a quiz this week, you must be able to identify each inner planet and give several facts for each.  So pay attention!!!!
Inner Planets. The inner planets are Mercury, Venus, Earth, and Mars. These planets get a lot of heat and light because they are close to the Sun. They.
The Inner Planets. Mercury Small Weak gravitational force No atmosphere Many craters.
 Small, have rocky surfaces  Terrestrial Planets: meaning earth.
SNC 1D. The Inner Planets  Terrestrial  Rocky iron core  High temperatures  Closer to the Sun  Closer to each other  Smaller than the outer planets.
Handout 27-3 The Inner Planets.
The Inner Planets. The terrestrial planets 1.Mercury 2. Venus 3. Earth 4.Mars.
Week 5 Notes Inner Planets Ch. 3, Sect. 3 Page 84 – 91.
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.
Chapter 27 Planets of the Solar System 27.3 The Inner Planets
THE INNER PLANETS The four planets that are closest to the sun are called the inner planets. They are all small and rocky. They are sometimes called the.
Section 3-1 (Part 2) Inner Planets.
The Inner Planets 20.3.
Chapter 9 The Terrestrial Planets. Mercury: The Messenger.
The Inner Planets Chapter Terrestrial Planets Mercury, Venus, Earth, Mars Mostly solid rock with metallic cores Impact craters.
The Inner Planets. The Inner Planets are:  Small: Compared to the Outer Planets  Rocky: Rocky surface – thin atmosphere  Dense: Heavy for their size.
The Inner Planets.
Chapter 9 The Terrestrial Planets. Mercury: The Messenger.
ROCK METAL CORE Inner Planets: Mercury, Venus, and Mars.
INNER PLANETS Terrestrial Planets are the Four planets closest to the sun. These planets have rocky terrain, and have higher temperatures due to receiving.
The Inner planets Section 28.2.
Chapter 29 The Solar System
Planet The International Astronomical Union (IAU) defines a planet as a body that: is in orbit around the sun has sufficient mass for its self-gravity.
What are the Inner planets?
Planetary Chart PlanetAUMassTypeAtmosphereMoons Mercury Venus Earth Mars Inner Planets Jupiter Saturn Uranus Neptune *Pluto.
Mars. When and where can you see it? Can be seen all night long. Sometimes undergoes apparent retrograde motion.
The Solar System.
By: Mrs. Crisp The Inner Planets S.P.I – Distinguish among the planets according to their known characteristics such as appearance, location,
Sept 29, 2003Astronomy 100 Fall 2003 Last Homework before Exam (HW#4) is due Friday at 11:50am. Nighttime observing has 8 more nights. Check the webpage.
The Solar System. Solar system – consists of the sun and, planets, and other objects that orbit the sun Nebular model – states that the sun and planets.
THE INNER PLANETS. WHAT DO THEY ALL HAVE IN COMMON? Q : Which planet is largest? Q : Which planet has the most moons? Q : Which planet is most similar.
The Terrestrial Planets Chapter 23, Section 2. Mercury: The Innermost Planet  Mercury, the innermost and smallest planet (not counting Pluto), is hardly.
Copyright © 2010 Pearson Education, Inc. The Terrestrial Planets.
27-3OBJECTIVES Identify the basic characteristics of the inner planets. Compare the characteristics of the inner planets. Summarize the features that allow.
Topic: The Inner Planets PSSA: D/S8.D.3.1. Objective: TLW explain how distance is measured in our solar system. TLW compare the characteristics.
The Terrestrial Planets Mercury, Venus, Earth, Mars.
The Inner Planets.
{ The Inner Planets Chapter 14 Section 3.
Terrestrial Planets (Chapter 17). Student Learning Objectives Identify & describe each Terrestrial Planet Compare & contrast the Terrestrial planets with.
The Inner Planets.
Planets in the Solar System
Norm Herr (sample file)
The Inner Planets Chapter 14.
Terrestrial Planets (Power Point 10) Image Credit: Space.com.
Section 3 – pg 552 The Inner Planets
Chapter 23 The Solar System
Section 3: The Inner Planets
Inner Planets.
Section 3: The Inner Planets
16-2 | The Inner Planets.
The Inner Planets of Our Solar System
The Inner Planets of Our Solar System
11-2 Inner Planets.
The Inner Planets Chapter 16-2.
16-2 | The Inner Planets.
Bell Ringer ________________ proposed the heliocentric model of the solar system? (S6E1a)   2. Explain the Geocentric Model of the Solar System.
Presentation transcript:

Chapter 27.3 The Inner Planets Std. 1a- Students know how the sun, the terrestrial planets, and the gas planets may have been established during the formation of the solar system Std. 4d- Students know the differing greenhouse conditions on Earth, Mars and Venus Objective 1: Identify the characteristics of the inner planets Objective 2: Summarize the features that allow Earth to sustain life

The Inner Planets Planets closest to the sun are: All similar to Earth Mercury 3. Earth Venus 4. Mars All similar to Earth Metallic cores and consist mostly of rock # of moons vary from 0-2

1) Mercury Planet closest to the sun (no moons) Orbits (day) the sun every 88 days Rotates (year) every 59 days Heavily cratered Slow rotation and no atmosphere causes a large temperature range (Day: 427°C and Night: -173°C) Orbit = day Rotates = year Made mostly of nickel and iron One the most dense planet in the solar system Very thin atmosphere Metric: 3.7 m/s2 English: 12.1 ft/s2 By Comparison: If you weigh 100 pounds on Earth, you would weigh 38 pounds on Mercury. Equatorial Circumference Metric: 15,329.1 km

2) Venus 2nd planet from the sun (no moons) Orbits the sun every 225 days Rotates every 243 days Same size, mass and density as Earth Hottest planet in the solar system Called the morning star because beside the moon it is the bright object in the sky Size: Equatorial circumference Metric: 38,024.6 km Earth: 40,030.2 km Density: Metric: 5.427 g/cm3 Earth = Metric: 5.513 g/cm3

Venus’s Atmosphere 96% carbon dioxide causing a greenhouse effect that heats the surface to 464 degrees C Hottest planet in the solar system Sulfur dioxide droplets in the upper atmosphere creates clouds which reflect sunlight It is the brightest object in the night sky (aside from the moon and sun) Atmosphere = Carbon Dioxide, Nitrogen Gravity Metric: 8.87 m/s2 English: 29.1 ft/s2 By Comparison: If you weigh 100 pounds on Earth, you would weigh 91 pounds on Venus.

Venus’s Surface Factors Venus rotates retrograde (east to west) compared with Earth's prograde (west to east) rotation.  On Earth, Jupiter and Saturn, lightning is associated with water clouds, but on Venus, it is associated with clouds of sulfuric acid. Venus is named for the ancient Roman goddess of love and beauty. (Venus is the Roman counterpart to the Greek goddess Aphrodite.) It is believed Venus was named for the most beautiful of the ancient gods because it shone the brightest of the five planets known to ancient astronomers It is thought that Venus was completely resurfaced by volcanic activity 300 to 500 million years ago. More than 1,000 volcanoes or volcanic centers larger than 20 km (12 miles) in diameter dot the surface. Has mountains, volcanoes, lava plains and sand dunes Lots of volcanic activity

Objective 1: Identify the characteristics of the inner planets How many moons do the inner planets have? 0-2 moons Which planet has the same mass and density as Earth? Venus What % of Venus’ s atmosphere is carbon dioxide? 96%

Earth 3rd planet from the sun (1 moon) Rotation 365 ¼ days Weathering and erosion continues to change Earth’s surface Earth's diameter is just a few hundred kilometers larger than that of Venus. We are enveloped by an atmosphere that consists of 78 percent nitrogen, 21 percent oxygen and 1 percent other ingredients.  The four seasons are a result of Earth's axis of rotation being tilted 23.45 degrees with respect to the plane of Earth's orbit around the sun. During part of the year, the northern hemisphere is tilted toward the sun and the southern hemisphere is tilted away, producing summer in the north and winter in the south. Our planet's rapid rotation and molten nickel-iron core give rise to a magnetic field, All of the planets, except for Earth, were named after Greek and Roman gods and goddesses. However, the name Earth is an English/German word, which simply means the ground: eor(th)e and ertha (Old English) and erde (German).

Water on Earth Life on Earth Atmosphere and distance from the sun allows water to exist in solid, liquid and gas states Life on Earth Earth maintained a moderate temperature during formation = it can support life

Mars 4th planet from the sun Orbital period 687 days Rotates every 24 hours 2 moons – Deimos and Phobos Same tilt as Earth – has similar seasons to Earth Equatorial circumference: 21,296.9 km Earth: 40,030.2 km Density: Metric: 3.934 g/cm3 Mass: 6.4169 x 1023 kg Gravity: Metric: 3.71 m/s2 English: 12.2 ft/s2 By Comparison: If you weigh 100 pounds on Earth, you would weigh 38 pounds on Mars. Mars is a rocky body about half the size of Earth.

Active volcanoes = unknown Seismic activity has been detected Martian Volcanoes Olympus Mons - Largest volcano is 3 times as tall as Mt. Everest The base is the size of Nebraska Reasons for large volcanoes - no moving tectonic plates Active volcanoes = unknown Seismic activity has been detected Mars was named by the Romans for their god of war because of its red, bloodlike color. Other civilizations also named this planet from this attribute; for example, the Egyptians named it "Her Desher," meaning "the red one." Volcanism was active more than 3 billion years ago, but some of the giant shield volcanoes are younger, having formed between 1 and 2 billion years ago. Mars has the largest volcanic mountain in the solar system, Olympus Mons, as well as a spectacular equatorial canyon system, Valles Marineris.

Mars Earth Water on Mars Pressure and temperature on Mars are too low for water to exist in liquid form Features caused by erosion indicate that water did exist in the past Water on Mars is trapped by polar icecaps Scientists believe that Mars experienced huge floods about 3.5 billion years ago. Though we do not know where the ancient flood water came from, how long it lasted or where it went, In 2002, NASA's Mars Odyssey orbiter detected hydrogen-rich polar deposits, indicating large quantities of water ice close to the surface. In 2004, the Mars Exploration Rover named Opportunity found structures and minerals indicating that liquid water was once present at its landing site. 

Objective 2: Summarize the features that allow Earth to sustain life Why can Earth support life? Earth maintained a moderate temperature during formation What is Mars’s largest volcano? Olympus Mons Why does Mars have large volcanoes? No moving tectonic plates Why can’t water on Mars exist in liquid form? Pressure and temperature is too low