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Chapter 18 review answers
Chapter 18 review answers

... 1. Astronomy is the study of all physical objects beyond Earth. P 482 2. Farmers looked to the sky to track the movements of the sun and stars and to determine when to plant. They looked at the constellations. P 482 3. The calendar is made up of days (24 hours), months (28-31 days) and the unit of a ...
Please jot down or ponder your answers. 1. What causes seasons
Please jot down or ponder your answers. 1. What causes seasons

... Using an arm’s length of register tape, each student will illustrate the relative distances between the orbits of the planets. 1. Write “Sun” on one end of the paper strip and “Pluto” on the other end. 2. Fold the tape in half; this is Uranus. Label the strip. 4. Fold Pluto to Uranus; this is Neptun ...
Wednesday, November 7, 2007
Wednesday, November 7, 2007

... pressure to resist gravity. • A hotter interior results in thermonuclear fusion proceeding more efficiently. Conversion of (stored) energy from mass into heat & light proceeds faster, so the star has a higher luminosity. We’re talking about the theory of the structure of a star here, because we are us ...
Astrophysics by Daniel Yang
Astrophysics by Daniel Yang

Cluster and Association Members
Cluster and Association Members

... are physically related groups of stars held together by mutual gravitational attraction. Therefore, they populate a limited region of space, which is typically much smaller than their distance from the Sun, so that the members are all approximately at the same distance. They are believed to originat ...
Objectives
Objectives

... • Less massive stars burn cooler and therefore can last longer • Our Sun will fuse hydrogen for about 10 billion years • Once a star’s Hydrogen supply runs out, fusion stops and the core begins to contract • At this time, the outer layers of hydrogen fuse at an incredible rate and the star expands t ...
The Sunspot Cycle
The Sunspot Cycle

... • Magnetic field produced in outer 30% of Sun’s radius. ...
Chapter 13 Exploring the final frontier
Chapter 13 Exploring the final frontier

... of interaction infinite. How are these same concepts viewed in the theory of relativity? 12. In one paragraph, describe what is meant by the ‘relativity of simultaneity’. 13. In terms of the energy required, accelerating a spacecraft to light speed is an impossibility. Explain why this is so. ...
E. Sci. Astronomy Notes
E. Sci. Astronomy Notes

... Meteor-Meteorite- Meteoroid Outer Gas Planets Jupiter, Saturn, Uranus, Neptune - all have “rings” Jupiter largest planet, gas giant, less dense Pluto/Charon and 10th Planet UB 313/moon are small, solid moon-like. Comets – “dirty snowballs”, huge elliptical orbits, tails point away due to solar wind ...
1 light year = 9 x 10 12 km
1 light year = 9 x 10 12 km

Characteristic Properties
Characteristic Properties

Is the Sun a Star? - Classroom Websites
Is the Sun a Star? - Classroom Websites

... school students, is to present new information about planetary systems that have been discovered around other stars. Students could begin by researching extrasolar planets at a website such as http:// planetquestjpl. nasa.gov! Having students draw what a distant planetary system might look like base ...
Stellar Evolution
Stellar Evolution

Document
Document

... The Photosphere • This is the origin of the 5,800 K thermal radiation we see. l = k/T = k/(5800 K)  l = 480 nm (visible light) • This is the light we see. • That’s why we see this as the “surface.” ...
HR DIAGRAM ACTIVITY
HR DIAGRAM ACTIVITY

... 4. Find the Sun on your HR diagram. Draw arrows on the HR diagram showing the various stages the Sun will go through until the end of its life cycle. (page 632) ...
The Sun - Ccphysics.us
The Sun - Ccphysics.us

... Sun will be blown off by the superwind created by the double shell burning in about 10,000 years • The very hot (but not enough for further fusion) core is revealed ...
The planets in the solar system
The planets in the solar system

... are formed during the collapse of a nebula into a thin disk of gas and dust. A proto-star (proto = early) forms at the core, surrounded by a rotating proto-planetary disk. Through a process called accretion (i.e., sticky collision) dust particles in the disk steadily accumulate mass to form ever-lar ...
Page pour l`impression
Page pour l`impression

... In the asteroid belt, it is well known that there are gaps, i.e. some zones where no objects are present. These locations are in resonance with Jupiter . The role of Jupiter has been to eject the bodies in resonance with the planet. The 3:2 resonance with Neptune plays the inverse role. At the locat ...
8.1 Stars
8.1 Stars

...  The area with the largest mass starts to pull more mass in. The matter pulled in has excess energy which causes the central ball of material to begin to spin. Extremely high pressures build up inside the ball, which in turn causes the tightly packed atoms to heat up. As the temperature climbs, the ...
Oceanography Chapter 1 – “Origins”
Oceanography Chapter 1 – “Origins”

... Nucleosynthesis of Light Elements • Hydrogen atoms: – the most common form of matter in the universe. • Atoms have mass. Clump together under gravity. • Formation of elements: – He through Fe (iron) inside stars (nuclear fusion) – Heavier elements in supernova explosion (Fe & beyond) ...
Measuring Time - BPS Science Weebly
Measuring Time - BPS Science Weebly

... Standard: 14 - Recognize that the earth revolves around (orbits) the sun in a year's time and that the earth rotates on its axis once approximately every 24 hours. Make connections between the rotation of the earth and day/night, and the apparent movement of the sun, moon, and stars across the sky. ...
Introduction to Astronomy
Introduction to Astronomy

... “We understand the possibility of determining [celestial bodies’] shapes, their distances, their sizes and motions, whereas never, by any means, will we be able to study their chemical composition. --Auguste Comte (philosopher), 1835 ...
Fingerprints in Starlight: Spectroscopy of Stars Inquiry Questions
Fingerprints in Starlight: Spectroscopy of Stars Inquiry Questions

... 6. Why is information about many stars contained in absorption rather than emission spectra? If there is a cloud of gas at a cooler temperature directly between a denser source producing a continuous spectrum (i.e. a star) and a telescope, the gas will absorb light at specific wavelengths that are c ...
What units are used in astronomical photometry?
What units are used in astronomical photometry?

... Distance: Distance is an easy concept to understand: it is just a length in some units such as in feet, km, light years, parsecs etc. It has been excrutiatingly difficult to measure astronomical distances until this century. Unfortunately most stars are so far away that it is impossible to directly ...
Electromagnetic Radiation from the Sun
Electromagnetic Radiation from the Sun

... 6. Why is information about many stars contained in absorption rather than emission spectra? If there is a cloud of gas at a cooler temperature directly between a denser source producing a continuous spectrum (i.e. a star) and a telescope, the gas will absorb light at specific wavelengths that are ...
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Aquarius (constellation)



Aquarius is a constellation of the zodiac, situated between Capricornus and Pisces. Its name is Latin for ""water-carrier"" or ""cup-carrier"", and its symbol is 20px (Unicode ♒), a representation of water.Aquarius is one of the oldest of the recognized constellations along the zodiac (the sun's apparent path). It was one of the 48 constellations listed by the 2nd century AD astronomer Ptolemy, and it remains one of the 88 modern constellations. It is found in a region often called the Sea due to its profusion of constellations with watery associations such as Cetus the whale, Pisces the fish, and Eridanus the river.
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