Powerpoint to Solar System Scale Activity by Doreen Jarvis
... Note: Use small print and do NOT use circles to represent objects! ...
... Note: Use small print and do NOT use circles to represent objects! ...
Unit 1
... – Instability comes from partial absorption of radiation in the interior of the star • Helium absorbs radiation, and the outer layers of the star get pushed away from core • As the star expands, the density decreases, letting photons escape • Outer layers head back inward toward core ...
... – Instability comes from partial absorption of radiation in the interior of the star • Helium absorbs radiation, and the outer layers of the star get pushed away from core • As the star expands, the density decreases, letting photons escape • Outer layers head back inward toward core ...
Chapter 11 Jovian Planet Systems Are jovian planets all alike
... much larger than Saturn even though it is three times more massive • Jovian planets with even more mass can be smaller than Jupiter ...
... much larger than Saturn even though it is three times more massive • Jovian planets with even more mass can be smaller than Jupiter ...
Slide 1
... would be about would equal about 510,000,000,000,000 miles (510 trillion miles or a diameter of about 84 light years!). ...
... would be about would equal about 510,000,000,000,000 miles (510 trillion miles or a diameter of about 84 light years!). ...
Answer Key Cloze
... Venus is the second planet from the Sun in our Solar System. It is the hottest planet in our Solar System. This planet is covered with fast-moving sulphuric acid clouds which trap heat from the Sun. Its thick atmosphere is mostly carbon dioxide. Its cloud cover traps the heat of the sun (the greenho ...
... Venus is the second planet from the Sun in our Solar System. It is the hottest planet in our Solar System. This planet is covered with fast-moving sulphuric acid clouds which trap heat from the Sun. Its thick atmosphere is mostly carbon dioxide. Its cloud cover traps the heat of the sun (the greenho ...
Science Jeopardy
... • ANSWER: These are the two gases that make up the majority of the outer planets’ atmospheres. • QUESTION: What are helium and ...
... • ANSWER: These are the two gases that make up the majority of the outer planets’ atmospheres. • QUESTION: What are helium and ...
Earth In Space - Hicksville Public Schools / Homepage
... OBJ: Given notes, video and activity sheet SWBAT explain the difference between rotation and revolution as well as what causes day and night with 70% accuracy DN: Distribute Astronomy Activity Sheet (w/ answer key); Astronomy Review Sheets (w/ answer key) ACT: Introduction to Rotation, Revolution (n ...
... OBJ: Given notes, video and activity sheet SWBAT explain the difference between rotation and revolution as well as what causes day and night with 70% accuracy DN: Distribute Astronomy Activity Sheet (w/ answer key); Astronomy Review Sheets (w/ answer key) ACT: Introduction to Rotation, Revolution (n ...
Celestial Sphere Lab
... (This lab has been modified from a University of Michigan Astronomy Department lab.) Introduction The ancient Greeks contributed much to the science of astronomy; however, many of the ideas they proposed have since proven to be incorrect. Some of the concepts they developed are still useful today th ...
... (This lab has been modified from a University of Michigan Astronomy Department lab.) Introduction The ancient Greeks contributed much to the science of astronomy; however, many of the ideas they proposed have since proven to be incorrect. Some of the concepts they developed are still useful today th ...
Solar Day and Sidereal Day for Mercury and Venus
... the picture as well and label how many Earth-days have passed. ...
... the picture as well and label how many Earth-days have passed. ...
Origin on the Space Weather on the Sun
... of solar coronal material that flows off the sun. Its consists of mostly electrons, protons and alpha particles with energies usually between 1.5 and 10 kEV The Earth's magnetic field acts as a shield for solar wind particles. However, there are regions of the ionosphere that are directly connected ...
... of solar coronal material that flows off the sun. Its consists of mostly electrons, protons and alpha particles with energies usually between 1.5 and 10 kEV The Earth's magnetic field acts as a shield for solar wind particles. However, there are regions of the ionosphere that are directly connected ...
V = 3 d3 = 4188.8 pc N = ρV = 0.1 pc χ 4188.8 pc = 419
... where M is the mass of the star. For what primary masses will any planets in the optimistic habitable zone be tidally locked? (Hint: Adopt the mass-luminosity relationship I showed in class to derive a relationship between the habitable zone distance and primary mass.) a) 0.11 MSun and below b) 0.25 ...
... where M is the mass of the star. For what primary masses will any planets in the optimistic habitable zone be tidally locked? (Hint: Adopt the mass-luminosity relationship I showed in class to derive a relationship between the habitable zone distance and primary mass.) a) 0.11 MSun and below b) 0.25 ...
Document
... g is the strength of the gravitational field at some point, then the gravitational force on an object of mass m at that point is Fgrav = mg. If g is the gravitational field strength at some point (in N/kg), then the free fall acceleration at that point is also g (in m/s2). ...
... g is the strength of the gravitational field at some point, then the gravitational force on an object of mass m at that point is Fgrav = mg. If g is the gravitational field strength at some point (in N/kg), then the free fall acceleration at that point is also g (in m/s2). ...
1 - Quia
... 21. What theory states that our universe formed from a large explosion of matter? (2 points) A. Moon Formation Theory B. Big Bang Theory ...
... 21. What theory states that our universe formed from a large explosion of matter? (2 points) A. Moon Formation Theory B. Big Bang Theory ...
gravitation_notes
... g is the strength of the gravitational field at some point, then the gravitational force on an object of mass m at that point is Fgrav = mg. If g is the gravitational field strength at some point (in N/kg), then the free fall acceleration at that point is also g (in m/s2). ...
... g is the strength of the gravitational field at some point, then the gravitational force on an object of mass m at that point is Fgrav = mg. If g is the gravitational field strength at some point (in N/kg), then the free fall acceleration at that point is also g (in m/s2). ...
New Worlds Ahead: The Discovery of Exoplanets
... eccentricity and i is the orbit inclination. The detailed modeling of the radial velocity curve vr (t) yields the measurement of P , as well as the eccentricity (distortion of vr (t) relative to a sinusoidal curve), the longitude and time of the passage at the periastron, and of K∗ . But as seen in ...
... eccentricity and i is the orbit inclination. The detailed modeling of the radial velocity curve vr (t) yields the measurement of P , as well as the eccentricity (distortion of vr (t) relative to a sinusoidal curve), the longitude and time of the passage at the periastron, and of K∗ . But as seen in ...
chapter11JovianPlane..
... • They are made up of numerous, tiny individual particles • They orbit over Saturn’s equator • They are very thin ...
... • They are made up of numerous, tiny individual particles • They orbit over Saturn’s equator • They are very thin ...
The Spring Night Sky – March, April and May All data sourced from
... The coming of spring heralds lighter nights and longer days. This limits some of the objects and constellations we can see but there are still some 'jewels' to be found in the night sky. March – all times in GMT The Moon First quarter Full moon Last quarter New moon ...
... The coming of spring heralds lighter nights and longer days. This limits some of the objects and constellations we can see but there are still some 'jewels' to be found in the night sky. March – all times in GMT The Moon First quarter Full moon Last quarter New moon ...
Solar System Tic Tac Toe
... Write the script for a short play detailing a conversation between 2 different celestial bodies. (Hint: The situation should be one where they have to describe themselves.) Act it out and submit the video on to the T-drive or on a USB. ...
... Write the script for a short play detailing a conversation between 2 different celestial bodies. (Hint: The situation should be one where they have to describe themselves.) Act it out and submit the video on to the T-drive or on a USB. ...
Gravitation
... The force always points from one particle to the other, so this equation can be written in vector form: Eq. (13-3) ...
... The force always points from one particle to the other, so this equation can be written in vector form: Eq. (13-3) ...
Document
... apparently formed near the beginning of the solar system. It is thus a “planetesimal”. ...
... apparently formed near the beginning of the solar system. It is thus a “planetesimal”. ...
PLANETS
... • In the Solar System, NOT same composition as Sun • Presence of gas implies formation while gas was still prevalent Cores: Gas giants may have a rocky or metallic core—in fact, such a core is thought to be required for a gas giant to form. H and He: The majority of its mass is in the form of the ga ...
... • In the Solar System, NOT same composition as Sun • Presence of gas implies formation while gas was still prevalent Cores: Gas giants may have a rocky or metallic core—in fact, such a core is thought to be required for a gas giant to form. H and He: The majority of its mass is in the form of the ga ...
Chapter 17 - Earth`s Place in Space
... Earth rotates on its axis and simultaneously revolves or orbits around the Sun. Which of these two motions is responsible for each of the following: ...
... Earth rotates on its axis and simultaneously revolves or orbits around the Sun. Which of these two motions is responsible for each of the following: ...
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.