Toilet Paper Solar System
... between the planets in our solar system. Voyager II, traveling at nearly 50,000 mph took 12 years to reach the planet Neptune! This gives you an idea of just how far our planets are from each other. However, we can make a scale model of the distances between the planets using almost anything as our ...
... between the planets in our solar system. Voyager II, traveling at nearly 50,000 mph took 12 years to reach the planet Neptune! This gives you an idea of just how far our planets are from each other. However, we can make a scale model of the distances between the planets using almost anything as our ...
Document
... • As the cloud continues to contract it begins to spin or orbit the center, which contains a YSO. The more it contracts the faster it spins. • Thus, a decrease in the size of a rotating mass must be balanced by an increase in its rotational speed. This concept is known as angular momentum and was fi ...
... • As the cloud continues to contract it begins to spin or orbit the center, which contains a YSO. The more it contracts the faster it spins. • Thus, a decrease in the size of a rotating mass must be balanced by an increase in its rotational speed. This concept is known as angular momentum and was fi ...
The Sun and Solar System - Dr. Alan F. Weekes` Website
... held together by gravity We are in the Milky Way Galaxy Named for the band of stars that stretches across the sky. ...
... held together by gravity We are in the Milky Way Galaxy Named for the band of stars that stretches across the sky. ...
SolarSystemScaleProject_05
... What inferences can you make based on this comparison? 4. Are the distances between the planets’ orbits spaced equally as you move outward from the Sun? Explain. 5. Is there any general trend in the distances between the planets’ orbits as you move outward from the Sun? If so, describe the trend. 6. ...
... What inferences can you make based on this comparison? 4. Are the distances between the planets’ orbits spaced equally as you move outward from the Sun? Explain. 5. Is there any general trend in the distances between the planets’ orbits as you move outward from the Sun? If so, describe the trend. 6. ...
Click here to view my classroom presentation
... •The Moon is the only natural satellite of Earth: •The Moon, of course, has been known since prehistoric times. It is the second brightest object in the sky after the Sun. •As the Moon orbits around the Earth once per month, the angle between the Earth, the Moon and the Sun changes; we see this as ...
... •The Moon is the only natural satellite of Earth: •The Moon, of course, has been known since prehistoric times. It is the second brightest object in the sky after the Sun. •As the Moon orbits around the Earth once per month, the angle between the Earth, the Moon and the Sun changes; we see this as ...
Fine structure of the interplanetary shocks observed by BMSW
... On the 9th September, 2011 five satellites - WIND, ACE, THEMIS-B, THEMIS-C and SPEKTR-R were simultaneously in the solar wind and consistently recorded the passage of an interplanetary shock wave. The position of satellites in space, in the interval 11:30 – 13:30 UT, shown on fig. 1.Using the locati ...
... On the 9th September, 2011 five satellites - WIND, ACE, THEMIS-B, THEMIS-C and SPEKTR-R were simultaneously in the solar wind and consistently recorded the passage of an interplanetary shock wave. The position of satellites in space, in the interval 11:30 – 13:30 UT, shown on fig. 1.Using the locati ...
Solar Interior
... • 1817 – Fraunhofer – solar spectral lines • 1907 – Hale – Zeeman splitting of spectral lines magnetic fields in sunspots. ...
... • 1817 – Fraunhofer – solar spectral lines • 1907 – Hale – Zeeman splitting of spectral lines magnetic fields in sunspots. ...
FROM COPERNICUS TO NEWTON TO EINSTEIN: TOWARD A
... insights will the next 35 years bring? At the heart of our planetary system is the Sun that controls our planetary destiny and which is slowly but inexorably converting hydrogen into helium and slowly losing mass. Measurements that could confirm the fundamental processes that govern our solar system ...
... insights will the next 35 years bring? At the heart of our planetary system is the Sun that controls our planetary destiny and which is slowly but inexorably converting hydrogen into helium and slowly losing mass. Measurements that could confirm the fundamental processes that govern our solar system ...
Solar System Webquest Go to http://www.kidsastronomy.com
... 3. The object pictured to the left can also be seen in the picture of the solar system. a. Identify this object _________________________ b. When is this object's "tail" visible? ____________ c. Which direction does its tail point (in reference to the sun)? ___________________ d. How does its orbit ...
... 3. The object pictured to the left can also be seen in the picture of the solar system. a. Identify this object _________________________ b. When is this object's "tail" visible? ____________ c. Which direction does its tail point (in reference to the sun)? ___________________ d. How does its orbit ...
Exercise G1: Our Home Galaxy, the Milky Way
... Question 3: The Sun is moving with a velocity of about 220 km/sec in its orbit about the galactic center. Using your answer from Question 2, what is the approximate time required for the Sun (and the entire Solar System) to complete one orbit of the galactic center? a. 115 million years b. 230 m ...
... Question 3: The Sun is moving with a velocity of about 220 km/sec in its orbit about the galactic center. Using your answer from Question 2, what is the approximate time required for the Sun (and the entire Solar System) to complete one orbit of the galactic center? a. 115 million years b. 230 m ...
Unit 14_EOC Review_4_23_Seasons_Lunar Cycle_tides
... I remember this information very well. I remember most of this information and only need to review a little. I remember a little over half of the information. I do need to review some of what I missed. I remember very little of this. I got a few questions right but I mostly guessed. I really need to ...
... I remember this information very well. I remember most of this information and only need to review a little. I remember a little over half of the information. I do need to review some of what I missed. I remember very little of this. I got a few questions right but I mostly guessed. I really need to ...
Review: sun spots and solar flares inner and outer planets what
... orbiting the sun beyond Neptune)and Oort Cloud (cloud of icy debris at the furthest reaches of suns gravity in our solar system) ...
... orbiting the sun beyond Neptune)and Oort Cloud (cloud of icy debris at the furthest reaches of suns gravity in our solar system) ...
1/ph/lb exploring the solar system
... Models of the Solar System: The geocentric system. The Copernican revolution and the heliocentric model. The origin and evolution of the Solar System, principally the nebular theory The Sun as a star, power source and structure. The solar magnetic environment, solar wind and the solar cycle. ...
... Models of the Solar System: The geocentric system. The Copernican revolution and the heliocentric model. The origin and evolution of the Solar System, principally the nebular theory The Sun as a star, power source and structure. The solar magnetic environment, solar wind and the solar cycle. ...
Unit 3 - Lesson 8.2 2011 Sun
... The sun rotates on its axis one time every 25 days. currents are caused as a heated material is forced away from the core while cooled materials fall back down. are darker, cooler areas visible on the sun’s photosphere are found in active regions and release large quantities of gas (big bulge) _____ ...
... The sun rotates on its axis one time every 25 days. currents are caused as a heated material is forced away from the core while cooled materials fall back down. are darker, cooler areas visible on the sun’s photosphere are found in active regions and release large quantities of gas (big bulge) _____ ...
ES1.Powerpoint.SolarSystem es1.powerpoint.solarsystem
... • 7th planet from sun • Covered with clouds • Uranus sits on its side with the north and south poles sticking out the sides. ...
... • 7th planet from sun • Covered with clouds • Uranus sits on its side with the north and south poles sticking out the sides. ...
Moons, Comets, Meteors, and Asteroids PowerPoint
... it close to the sun, it heats up and spews dust and gas into a giant glowing head, which then forms a tail that stretches away from the sun for millions of kilometers. What does a passing comet sound like? Click here to find out! ...
... it close to the sun, it heats up and spews dust and gas into a giant glowing head, which then forms a tail that stretches away from the sun for millions of kilometers. What does a passing comet sound like? Click here to find out! ...
8th Grade Earth Science State and District Outcomes Summary
... 2. Earth has a variety of climates defined by average temperature, precipitation, humidity, air pressure, and wind that have changed over time in a particular location 3.2a Develop, communicate and justify an evidence-based scientific explanation to account for Earth’s different climates 3.2b Resear ...
... 2. Earth has a variety of climates defined by average temperature, precipitation, humidity, air pressure, and wind that have changed over time in a particular location 3.2a Develop, communicate and justify an evidence-based scientific explanation to account for Earth’s different climates 3.2b Resear ...
here
... • Many of these are “changes” of the Earth • Students consider the Sun itself to be pretty constant. – Not a bad assumption but certainly not correct – Solar Constant: 1300 - 1400 W/m2 ...
... • Many of these are “changes” of the Earth • Students consider the Sun itself to be pretty constant. – Not a bad assumption but certainly not correct – Solar Constant: 1300 - 1400 W/m2 ...
ASTR 241 syllabus Barnes
... This course introduces students to the Solar System as an arena for physics, and teaches them to solve Solar System problems by applying basic physical laws. Students passing this course will be able to calculate orbital trajectories of planets and other objects, evaluate surface temperatures for pl ...
... This course introduces students to the Solar System as an arena for physics, and teaches them to solve Solar System problems by applying basic physical laws. Students passing this course will be able to calculate orbital trajectories of planets and other objects, evaluate surface temperatures for pl ...
Griffith Park Observatory
... Choose one exhibit and write a one paragraph explanation of the science behind the exhibit. a. Physics students: choose an exhibit related to forces, motion, energy, momentum, heat, thermodynamics, waves, or electricity and magnetism. Suggestions include: Extending the Eye, Beyond the Visible, Tesla ...
... Choose one exhibit and write a one paragraph explanation of the science behind the exhibit. a. Physics students: choose an exhibit related to forces, motion, energy, momentum, heat, thermodynamics, waves, or electricity and magnetism. Suggestions include: Extending the Eye, Beyond the Visible, Tesla ...
Labs/Teacher Notes Solar System to Scale Outside
... Our galaxy would be 3.9 million miles across at this scale! 3. Starting the activity I give students pictures representing the various objects including the Sun. Outside I then have the students stand at the appropriate places and say the rotation and revolution rate for each planet. 4. I also demon ...
... Our galaxy would be 3.9 million miles across at this scale! 3. Starting the activity I give students pictures representing the various objects including the Sun. Outside I then have the students stand at the appropriate places and say the rotation and revolution rate for each planet. 4. I also demon ...
Activity Voyager Key Learning Students will develop their
... 8 – Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus and Neptune. Sun – the sun is the star at the centre of the solar system. Mercury – Mercury is the smallest and closest planet to the sun. 4.6 billion years ago – scientists believe that the solar system evolved from a giant cloud of dust and ...
... 8 – Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus and Neptune. Sun – the sun is the star at the centre of the solar system. Mercury – Mercury is the smallest and closest planet to the sun. 4.6 billion years ago – scientists believe that the solar system evolved from a giant cloud of dust and ...
Heliosphere
The heliosphere is the bubble-like region of space dominated by the Sun, which extends far beyond the orbit of Pluto. Plasma ""blown"" out from the Sun, known as the solar wind, creates and maintains this bubble against the outside pressure of the interstellar medium, the hydrogen and helium gas that permeates the Milky Way Galaxy. The solar wind flows outward from the Sun until encountering the termination shock, where motion slows abruptly. The Voyager spacecraft have actively explored the outer reaches of the heliosphere, passing through the shock and entering the heliosheath, a transitional region which is in turn bounded by the outermost edge of the heliosphere, called the heliopause. The overall shape of the heliosphere is controlled by the interstellar medium, through which it is traveling, as well as the Sun, and does not appear to be perfectly spherical. The limited data available and unexplored nature of these structures have resulted in many theories.On September 12, 2013, NASA announced that Voyager 1 had exited the heliosphere on August 25, 2012, when it measured a sudden increase in plasma density of about forty times. Because the heliopause marks one boundary between the Sun's solar wind and the rest of the galaxy, a spacecraft such as Voyager 1 which has departed the heliosphere can be said to have reached interstellar space.