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Monday – October 29th - East Hanover Township School District
Monday – October 29th - East Hanover Township School District

Constellations
Constellations

... › If all were placed at same distance from ...
Exoplanets. I
Exoplanets. I

... Planets do not orbit the Sun - they both orbit the center of mass. The radius of the orbit is inversely proportional to the mass The radius of the Sun’s orbit with respect to the Earth is 1/300,000 AU, or 500 km R 1 M1 = R 2 M 2 ...
IV. ASTRONOMY: THE SUN and the MOON
IV. ASTRONOMY: THE SUN and the MOON

... shift of stars at the edge of the Sun was 1.7 seconds of arc, as predicted by the stars. f. New of the confirmation made Einstein an instant celebrity; before this he was still obscure, at least to the lay public. g. Measurements during subsequent eclipses were used to confirm the predicted bending. ...
1.1 Organization of the Universe
1.1 Organization of the Universe

... Darnell wants to see if flies like honey or vinegar more. He puts out two bowls: one of honey, one of vinegar. Then, he counts how many flies land on each bowl.  What ...
Our Star, the Sun Chapter Eighteen Guiding Questions
Our Star, the Sun Chapter Eighteen Guiding Questions

... What is the source of the Sun’s energy? What is the internal structure of the Sun? How can astronomers measure the properties of the Sun’s interior? 4. How can we be sure that thermonuclear reactions are happening in the Sun’s core? 5. Does the Sun have a solid surface? 6. Since the Sun is so bright ...
Document
Document

... What is the source of the Sun’s energy? What is the internal structure of the Sun? How can astronomers measure the properties of the Sun’s interior? 4. How can we be sure that thermonuclear reactions are happening in the Sun’s core? 5. Does the Sun have a solid surface? 6. Since the Sun is so bright ...
The Sun The Sun
The Sun The Sun

Don`t Panic, But the Sun Will (Far) Outlive Earth (Op-Ed)
Don`t Panic, But the Sun Will (Far) Outlive Earth (Op-Ed)

... This 10% increase in the sun’s brightness, triggering the evaporation of our oceans, will occur over the next billion years or so. Predictions of exactly how rapidly this process will unfold depend on who you talk to. Most models suggest that as the oceans evaporate, more and more water will be pres ...
PH2213 : Examples from Chapter 6 : Gravitation Key Concepts Two
PH2213 : Examples from Chapter 6 : Gravitation Key Concepts Two

... The radius of the Earth is about 6380 km so the point that both the Earth and Moon are circling is located about 1/4 of radius of the Earth underground. This results in the Earth ‘wobbling’ with a roughly 30 day period as it orbits the Sun. You can apply the same process to other pairs of objects. ...
(Sol) Basic information Sun “Sol” Size
(Sol) Basic information Sun “Sol” Size

... • "like" full moon CLICKER: The corona is so dim relative to the photosphere because…? (a)  most of the emission is not in visible light (b)  the density is very low (c)  it is colder than the photosphere (d)  magnetic field lines cannot trap the hot gas (e)  both a & b (f) both b & c (g) both c & d ...
Modeling axial tilt and daylight
Modeling axial tilt and daylight

... Daylight period over the course of the year Keep your Earth’s axis pointed at your “North Star,” and move to a different place around your model Sun. This simulates a different time of year (since the Earth is at a different place in its orbit). Simulate a “day” by spinning your Earth counter-clockw ...
The Hertzsprung-Russell diagram and the nature of stars
The Hertzsprung-Russell diagram and the nature of stars

... How can we know the structure of the Sun below the photosphere? • Application of the laws of physics (equations of stellar structure), find solution consistent with mass and radius of Sun • Measure “eigenmodes” of the Sun (see how fast it jiggles • Results for how the sun is put together ...
The Big Bang
The Big Bang

... Expansion of the Universe • In 1929 Edwin Hubble found link between distances to galaxies and their radial velocities • Plot Hubble's data ...
Earth
Earth

... But that is small comfort. In its retirement from normal core fusion, our previously nurturing star will care little for its planetary children. It will be pumping out a thousand times more energy, making Earth a good approximation to hell. To add insult to injury, the solar wind -- a stream of par ...
Earth at Aphelion - Stargazers Lounge
Earth at Aphelion - Stargazers Lounge

... Having a great July 4th? The day gives us another cause to celebrate, as the Earth reaches aphelion today, or our closest point to our host star. Aphelion is the opposite of the closest point of the year, known as perihelion. Note that the ‘helion’ part only applies to things in solar orbit, perigee ...
The Seasons Interactive - Home
The Seasons Interactive - Home

Solar System.3rd.Mark Vega
Solar System.3rd.Mark Vega

... out circle) counterclockwise direction. The inner planets orbit much faster then the outer planets. Venus is the one inner planet that has a different rotation – it rotates in a clockwise rotation while all the other inner planets rotate in a counter-clockwise direction. The outer planets all rotate ...
Section 1
Section 1

... koh BRAH uh) and his assistants made much more accurate observations. For more than 20 years, they carefully observed and recorded the positions of the planets. Surprisingly, these observations were made without using a telescope. Telescopes had not yet been invented! Kepler’s Calculations Tycho Bra ...
Unit 2 Section 1
Unit 2 Section 1

... koh BRAH uh) and his assistants made much more accurate observations. For more than 20 years, they carefully observed and recorded the positions of the planets. Surprisingly, these observations were made without using a telescope. Telescopes had not yet been invented! Kepler’s Calculations Tycho Bra ...
Peer Instruction/Active Learning
Peer Instruction/Active Learning

... 2)  Peer  Instruc#on:    Ten  years  of  experience  and  results,  Catherine  H.  Crouch  and  Eric  Mazur,  Am.  J.  Phys.  69,   ...
TENTH GRADE SCOPE AND SEQUENCE DRAFT
TENTH GRADE SCOPE AND SEQUENCE DRAFT

The Sun (Nearest Star to us)
The Sun (Nearest Star to us)

... An H-alpha filtergram reveals that the chromosphere contain complex structure which is invisible in normal ...
Introduction to Astronomy
Introduction to Astronomy

... 1. If it’s a summer day here, what season and time of day is it in Russia? Russia would be summer night 2. If it’s a winter night here, what season and time of day is it in Peru? Peru would be summer night 3. If it’s a summer night here, what season and time of day is it in Australia? Australia woul ...
Size of Sun and Size of Planets
Size of Sun and Size of Planets

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Astronomical unit

The astronomical unit (symbol au, AU or ua) is a unit of length, roughly the distance from the Earth to the Sun. However, that distance varies as the Earth orbits the Sun, from a maximum (aphelion) to a minimum (perihelion) and back again once a year. Originally conceived as the average of Earth's aphelion and perihelion, it is now defined as exactly 7011149597870700000♠149597870700 meters (about 150 million kilometers, or 93 million miles). The astronomical unit is used primarily as a convenient yardstick for measuring distances within the Solar System or around other stars. However, it is also a fundamental component in the definition of another unit of astronomical length, the parsec.
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