RAFT Idea Space Stuff to Scale
... better represent the planets and Moon.) (Scale: 1 cm = 2550 km) 2. Place the Earth ball on a large table. Predict where the Moon would be if the Earth were that size. 3. The Moon is 400,000 km from Earth (on average), 155 cm at the scale in this activity. Measure 155 cm from the Earth ball, and plac ...
... better represent the planets and Moon.) (Scale: 1 cm = 2550 km) 2. Place the Earth ball on a large table. Predict where the Moon would be if the Earth were that size. 3. The Moon is 400,000 km from Earth (on average), 155 cm at the scale in this activity. Measure 155 cm from the Earth ball, and plac ...
Solar System Scale - Siemens Science Day
... moon mainly because it is heavily cratered. The side that faces the sun is extremely hot, but the opposite side is extremely cold. The MESSENGER mission has recently discovered that water deposits are hidden deep within the dark craters of Mercury. Mercury is now the smallest planet in our solar sys ...
... moon mainly because it is heavily cratered. The side that faces the sun is extremely hot, but the opposite side is extremely cold. The MESSENGER mission has recently discovered that water deposits are hidden deep within the dark craters of Mercury. Mercury is now the smallest planet in our solar sys ...
Chapter 6 Solar System Chapter Test Lesson 1 Sun Aurora borealis
... 1. The four planets closest to the sun are called the _____ planets. 2. These 4 planets (in order from closest to the Sun) are _____, _____, _____, and _____. 3. The four planets farthest from the sun are called the _____ planets. 4. These 4 planets (in order from closest to the sun) are _____. ____ ...
... 1. The four planets closest to the sun are called the _____ planets. 2. These 4 planets (in order from closest to the Sun) are _____, _____, _____, and _____. 3. The four planets farthest from the sun are called the _____ planets. 4. These 4 planets (in order from closest to the sun) are _____. ____ ...
Nebular theory
... Our theory about how the solar system formed is called the nebular theory. This activity will help you understand how we think the solar system formed. 1. Write your observations from the video that shows how the planets orbit the sun. Write at least 4 observations. Look for similarities, difference ...
... Our theory about how the solar system formed is called the nebular theory. This activity will help you understand how we think the solar system formed. 1. Write your observations from the video that shows how the planets orbit the sun. Write at least 4 observations. Look for similarities, difference ...
Our Solar System
... A non-satellite body fulfilling only the first two of these criteria is classified as a "dwarf planet", whilst a non-satellite body fulfilling only the first criterion is termed a "small solar system body" (SSSB). The definition was a controversial one, and has drawn both support and criticism from ...
... A non-satellite body fulfilling only the first two of these criteria is classified as a "dwarf planet", whilst a non-satellite body fulfilling only the first criterion is termed a "small solar system body" (SSSB). The definition was a controversial one, and has drawn both support and criticism from ...
Astronomy Assignment #1
... the Sun in Astronomical Units, density in g/cm3, mass in Earth masses, radius in Earth radii, nature of the surface, principle composition and depth (shallow or deep)* of the atmosphere, number of natural satellites, rotation period in days (Ignore negative signs) The information can be obtained fro ...
... the Sun in Astronomical Units, density in g/cm3, mass in Earth masses, radius in Earth radii, nature of the surface, principle composition and depth (shallow or deep)* of the atmosphere, number of natural satellites, rotation period in days (Ignore negative signs) The information can be obtained fro ...
4QA Jeopardy
... One piece of evidence used to back up the Big Bang was the Doppler Effect. What does the Doppler Affect show us? a.) Stars and Galaxies are moving away ...
... One piece of evidence used to back up the Big Bang was the Doppler Effect. What does the Doppler Affect show us? a.) Stars and Galaxies are moving away ...
(the inner and outer planets).
... •Pluto is small compared to the other outer planets. •Pluto is composed of rock compared to the “gas giants.” •Pluto does not have any rings. ...
... •Pluto is small compared to the other outer planets. •Pluto is composed of rock compared to the “gas giants.” •Pluto does not have any rings. ...
How Many Regions Are There In The Solar System?
... wealth of the asteroid belt is 100 billion dollars for every person on Earth today The average surface temperature of an asteroid is -73C (-100F) ...
... wealth of the asteroid belt is 100 billion dollars for every person on Earth today The average surface temperature of an asteroid is -73C (-100F) ...
Powerpoint 2003
... Galileo discovered that the higher an object is dropped, the greater its speed when it reaches the ground All falling objects near the surface of the Earth have the same acceleration (9.8 m/s2) The acceleration of gravity on the surface of other solar-system bodies depends on their mass and radius • ...
... Galileo discovered that the higher an object is dropped, the greater its speed when it reaches the ground All falling objects near the surface of the Earth have the same acceleration (9.8 m/s2) The acceleration of gravity on the surface of other solar-system bodies depends on their mass and radius • ...
Astronomy: Week #5 Assignment
... 5. How does the interior of Jupiter differ from the interior of the Earth? 6. Given that Jupiter’s diameter is 11.2 times that of Earth, about how many Earths could fit inside of Jupiter? 7. Contrast the volcanoes of Io with those of Earth. 8. Compare the surfaces of Callisto, Io, and Earth’s Moon. ...
... 5. How does the interior of Jupiter differ from the interior of the Earth? 6. Given that Jupiter’s diameter is 11.2 times that of Earth, about how many Earths could fit inside of Jupiter? 7. Contrast the volcanoes of Io with those of Earth. 8. Compare the surfaces of Callisto, Io, and Earth’s Moon. ...
Planets of the Solar System Information
... The four largest moons, called Io, Europa, Ganymede and Callisto were discovered by Galileo Gallilei in 1610 with the newly invented telescope. Ganymede, Jupiter’s largest moon, is bigger than Mercury. Jupiter’s most striking features are its swirling red spot which is shaped like an eye and its clo ...
... The four largest moons, called Io, Europa, Ganymede and Callisto were discovered by Galileo Gallilei in 1610 with the newly invented telescope. Ganymede, Jupiter’s largest moon, is bigger than Mercury. Jupiter’s most striking features are its swirling red spot which is shaped like an eye and its clo ...
Chapter 27 Stars and Galaxies
... III. Star Groups A. Constellations: patterns of stars in the sky there are 88 different patterns of stars recognized. ...
... III. Star Groups A. Constellations: patterns of stars in the sky there are 88 different patterns of stars recognized. ...
Life in the Universe Lecture (G 345U)
... Key Point 1) formation of Earth and solar system is byproduct of our sun forming, -Involves Astronomy, Meteorites, and planetary science. Meteorites are the building blocks and planetary science for comparison among various planets. Key concept: Planetary systems form as a byproduct of star formatio ...
... Key Point 1) formation of Earth and solar system is byproduct of our sun forming, -Involves Astronomy, Meteorites, and planetary science. Meteorites are the building blocks and planetary science for comparison among various planets. Key concept: Planetary systems form as a byproduct of star formatio ...
Chpt 27 Notes
... 2. Explain what a dwarf planet is. A dwarf planet is a protoplanet that is still in the developmental process and has not met the two requirements of a plant. The first requirement is that the object has coalesced into a globe shaped object (their shape is not oblong or random like an asteroid). The ...
... 2. Explain what a dwarf planet is. A dwarf planet is a protoplanet that is still in the developmental process and has not met the two requirements of a plant. The first requirement is that the object has coalesced into a globe shaped object (their shape is not oblong or random like an asteroid). The ...
Life Cycle of a Star Notes
... together to form heavier elements such as helium and release energy. If enough matter is left behind, this may be so dense, and its gravitational field so strong that nothing can escape from it, not even light or other forms of electromagnetic radiation. It is then called a black hole. We cannot see ...
... together to form heavier elements such as helium and release energy. If enough matter is left behind, this may be so dense, and its gravitational field so strong that nothing can escape from it, not even light or other forms of electromagnetic radiation. It is then called a black hole. We cannot see ...
Quiz # 1 - Oglethorpe University
... C) path traced out by the Moon in our sky in one month against the background stars. D) path traced out by the Sun in our sky over one year against the background stars. ...
... C) path traced out by the Moon in our sky in one month against the background stars. D) path traced out by the Sun in our sky over one year against the background stars. ...
Astronomy 101 Section 4
... Our tour continues with a visit to the nearest galaxies - here the Large Magellanic Cloud. ...
... Our tour continues with a visit to the nearest galaxies - here the Large Magellanic Cloud. ...
Sorting the Solar System - California Academy of Sciences
... 2. Explain that scientists sort things by their characteristics – size, composition, position ...
... 2. Explain that scientists sort things by their characteristics – size, composition, position ...
Mathematical Relationships of Solar System Bodies revealed using
... Thus it is to be expected that a (faint) disc of some sort would develop about the Sun. The T-Tauri mechanism together with centrifuge separation of matter within the molecular (?) cloud gives a simple explanation for the Solar System’s 18O being uniquely higher (+40%) than that of our galaxy. 2. As ...
... Thus it is to be expected that a (faint) disc of some sort would develop about the Sun. The T-Tauri mechanism together with centrifuge separation of matter within the molecular (?) cloud gives a simple explanation for the Solar System’s 18O being uniquely higher (+40%) than that of our galaxy. 2. As ...
Article - public.iastate.edu
... Now he said he is working on furthering debate by encouraging online discussions on what the characteristics of a planet should be with the goal of creating a definition more effective than the union's. Pluto's planet status has eroded since its discovery in 1930, and it has been found to be far les ...
... Now he said he is working on furthering debate by encouraging online discussions on what the characteristics of a planet should be with the goal of creating a definition more effective than the union's. Pluto's planet status has eroded since its discovery in 1930, and it has been found to be far les ...
“The Big Bang”- The Life Cycle of the Sun
... This is can be used as a KWL. Go over some thoughts about what we do know already about space? Ex: The sun is a star. Discuss why the sun is important to us. Discuss why the sun looks so much larger and brighter than other stars. Use models to explain relative size and distance. ( some examples in h ...
... This is can be used as a KWL. Go over some thoughts about what we do know already about space? Ex: The sun is a star. Discuss why the sun is important to us. Discuss why the sun looks so much larger and brighter than other stars. Use models to explain relative size and distance. ( some examples in h ...
A Tour of our Solar System
... Saturn Saturn's rings are made mostly of dust and rocks the size of a baseball or smaller. There has been a lot of study done to understand why they exist. The jury is still out, but there are ideas about gravity and Saturn’s magnetic field. ...
... Saturn Saturn's rings are made mostly of dust and rocks the size of a baseball or smaller. There has been a lot of study done to understand why they exist. The jury is still out, but there are ideas about gravity and Saturn’s magnetic field. ...
History of Solar System formation and evolution hypotheses
Ideas concerning the origin and fate of the world date from the earliest known writings; however, for almost all of that time, there was no attempt to link such theories to the existence of a ""Solar System"", simply because almost no one knew or believed that the Solar System, in the sense we now understand it, existed. The first step towards a theory of Solar System formation was the general acceptance of heliocentrism, the model which placed the Sun at the centre of the system and the Earth in orbit around it. This conception had been gestating for thousands of years, but was only widely accepted by the end of the 17th century. The first recorded use of the term ""Solar System"" dates from 1704.