Astronomy 10: Introduction to General Astronomy Instructor: Tony
... must be true according to Newton’s 3rd law, but also it is apparent from Newton’s law of gravitation because the gravitational force, F = Gm1 m2 /d2 does not change if we exchange 1 and 2. (12) page 109, question 28, Even though it is multiple choice, be sure to show your work From Kepler’s 3rd law, ...
... must be true according to Newton’s 3rd law, but also it is apparent from Newton’s law of gravitation because the gravitational force, F = Gm1 m2 /d2 does not change if we exchange 1 and 2. (12) page 109, question 28, Even though it is multiple choice, be sure to show your work From Kepler’s 3rd law, ...
The Sun
... If the Sun did not exist, there would be no life on Earth. The Sun plays vital roles in most of the processes on Earth, as well as in every life on Earth. The Sun provides plants with energy for photosynthesis. It is also the basis for birds’ migration schedules. Sunlight is even the essential ingre ...
... If the Sun did not exist, there would be no life on Earth. The Sun plays vital roles in most of the processes on Earth, as well as in every life on Earth. The Sun provides plants with energy for photosynthesis. It is also the basis for birds’ migration schedules. Sunlight is even the essential ingre ...
Ch. 2
... Anything that can fly this fast will not hit the ground. This is the speed for low Earth orbital objects like the Space Shuttle, the ISS (International Space Station) and spy satellites. ...
... Anything that can fly this fast will not hit the ground. This is the speed for low Earth orbital objects like the Space Shuttle, the ISS (International Space Station) and spy satellites. ...
The Solar System: Cosmic encounter with Pluto
... Calculate: In July 2015, when the New Horizons space probe flies past Pluto, the Earth will be 4,920,000,000 km away. Calculate this distance in AU. ...
... Calculate: In July 2015, when the New Horizons space probe flies past Pluto, the Earth will be 4,920,000,000 km away. Calculate this distance in AU. ...
space - jennseymour
... wobbles a bit as time goes by Right now, our axis points towards the North Star, also known as Polaris. Someday, the axis will point towards ...
... wobbles a bit as time goes by Right now, our axis points towards the North Star, also known as Polaris. Someday, the axis will point towards ...
Sun 1 - Prescott Astronomy Club
... the sky. The glow stretched from the horizon to approximately the "W" of the constellation Cassiopeia and was about 30 to 40 degrees wide. Also, there were a couple of vertical 'zones' in the glow. The glow could be observed through the car windows for about 5 minutes, but by the time we reached the ...
... the sky. The glow stretched from the horizon to approximately the "W" of the constellation Cassiopeia and was about 30 to 40 degrees wide. Also, there were a couple of vertical 'zones' in the glow. The glow could be observed through the car windows for about 5 minutes, but by the time we reached the ...
Distance - courses.psu.edu
... 1/10,000 (one ten-thousandth) the Sun's flux. What would be the distance to this star, in AU? 7. Two stars, A and B, are known to be equal in luminosity, but A appears 16 times brighter (as viewed from Earth) than B. Which one is more distant, and how much farther away is it than the other? 8. Tripl ...
... 1/10,000 (one ten-thousandth) the Sun's flux. What would be the distance to this star, in AU? 7. Two stars, A and B, are known to be equal in luminosity, but A appears 16 times brighter (as viewed from Earth) than B. Which one is more distant, and how much farther away is it than the other? 8. Tripl ...
Rotation and Revolution
... around a star. The sun is the star of our solar system and controls the motion of all the planets that travel around it. The planets are illuminated, or lit up, by sunlight. Some planets may be mistaken as bright stars on a clear night. However, when carefully observed, planets shine with a steady g ...
... around a star. The sun is the star of our solar system and controls the motion of all the planets that travel around it. The planets are illuminated, or lit up, by sunlight. Some planets may be mistaken as bright stars on a clear night. However, when carefully observed, planets shine with a steady g ...
Star Patterns - Lincoln-Sudbury Regional High School
... You may have noticed that the dates corresponding to each zodiacal constellation are not the same as the dates commonly quoted for “star signs”. In the next Activity, we will investigate why this is so. Another question may have occurred to you: For example, when the Sun is “in” Aquarius, Aquarius ...
... You may have noticed that the dates corresponding to each zodiacal constellation are not the same as the dates commonly quoted for “star signs”. In the next Activity, we will investigate why this is so. Another question may have occurred to you: For example, when the Sun is “in” Aquarius, Aquarius ...
The Life of a Star
... a red super giant. After this stage things become more violent. Instead of gentle billowing gas shells being ejected into space (a planetary nebula) the red super giant tears itself apart in an unbelievably violent explosion called a supernova. As the radiation and debris clear, a neutron star emerg ...
... a red super giant. After this stage things become more violent. Instead of gentle billowing gas shells being ejected into space (a planetary nebula) the red super giant tears itself apart in an unbelievably violent explosion called a supernova. As the radiation and debris clear, a neutron star emerg ...
The Solar System
... Example: Because the Moon has so much less mass than the Earth, there is much less gravitational pull on the Moon than on the Earth, therefore, you would weigh less on the Moon and have a much easier time jumping into the air. [However, your mass will remain the same because you didn’t change the am ...
... Example: Because the Moon has so much less mass than the Earth, there is much less gravitational pull on the Moon than on the Earth, therefore, you would weigh less on the Moon and have a much easier time jumping into the air. [However, your mass will remain the same because you didn’t change the am ...
Solar evolution and the distant future of Earth
... have used the definition of the effective temthe encounter would be too brief to cause any perature of the Sun, L = 4πRSun2 σTSun4 . significant orbital change. In fact, we do not For the present Sun, this gives a mean temresolve thermal pulses for reasons of simplicity perature for the Earth (assum ...
... have used the definition of the effective temthe encounter would be too brief to cause any perature of the Sun, L = 4πRSun2 σTSun4 . significant orbital change. In fact, we do not For the present Sun, this gives a mean temresolve thermal pulses for reasons of simplicity perature for the Earth (assum ...
Star and Sun Properties
... • The Sun, our closest star, is 93 million miles from Earth. • The next closest star is 4.3 lighter years away. • By mass, the Sun is 71 % Hydrogen, 27% helium and the rest heavier element. This is similar to the composition of the universe. • The Sun is about 4.6 billion years old. ...
... • The Sun, our closest star, is 93 million miles from Earth. • The next closest star is 4.3 lighter years away. • By mass, the Sun is 71 % Hydrogen, 27% helium and the rest heavier element. This is similar to the composition of the universe. • The Sun is about 4.6 billion years old. ...
Planisphere Exercise
... In what direction does the celestial equator appear to “rise” and “set” as the night progresses? Do these directions ever change? Turn the star wheel to find out. ...
... In what direction does the celestial equator appear to “rise” and “set” as the night progresses? Do these directions ever change? Turn the star wheel to find out. ...
Name________________________________________
... releasing __________ and _______________. Clouds of gas and dust form a fuzzy outer layer called a _______________. A comet’s coma has a solid inner core called a ____________________. The nucleus and coma (the comet’s head) is the _________________________ part of a comet. The comet’s tail… As a co ...
... releasing __________ and _______________. Clouds of gas and dust form a fuzzy outer layer called a _______________. A comet’s coma has a solid inner core called a ____________________. The nucleus and coma (the comet’s head) is the _________________________ part of a comet. The comet’s tail… As a co ...
Lecture 3
... seasons come back to later for stars • Geocentric parallax uses the earth as a base. • Make a measurement two or more times in one night. • Use for planets/Sun/Moon Brahe’s data also had distances to planets plus position in sky 162 Class 3 ...
... seasons come back to later for stars • Geocentric parallax uses the earth as a base. • Make a measurement two or more times in one night. • Use for planets/Sun/Moon Brahe’s data also had distances to planets plus position in sky 162 Class 3 ...
Lesson #5: Constellations - Center for Learning in Action
... different types of stars. Ask students if they have ever seen any of these stars before. Ask the students what a formation of stars is called. Stars in a pattern are called a constellation. Give them examples such as the Big or Little ...
... different types of stars. Ask students if they have ever seen any of these stars before. Ask the students what a formation of stars is called. Stars in a pattern are called a constellation. Give them examples such as the Big or Little ...
Problem set 1 solution
... In reality, the local times will be somewhat less than this: 22h 59m and 6h 59m . The main difference arises because local noon at Greenwich does not correspond exactly to 0h UT on the vernal equinox, as was assumed. UT is designed so that this correspondence holds on the average, but it will not be ...
... In reality, the local times will be somewhat less than this: 22h 59m and 6h 59m . The main difference arises because local noon at Greenwich does not correspond exactly to 0h UT on the vernal equinox, as was assumed. UT is designed so that this correspondence holds on the average, but it will not be ...
PHYS 2410 General Astronomy Homework 5
... I. the latitude at which sunspots are visible at a given time. II. the number of sunspots that are visible at a given time. III. the rotation rate of the sun's equator at a given time. ...
... I. the latitude at which sunspots are visible at a given time. II. the number of sunspots that are visible at a given time. III. the rotation rate of the sun's equator at a given time. ...
SylTerNav\4Curr\emet
... orbit and the stability of the axis (ignoring precession) and show how it causes the seasons; 7.1.5 state the dates of the solstices and equinoxes; 7.1.6 explain the concept of the earth's axial rotation causing day and night; 7.1.7 explain what causes the varying length of daylight through the year ...
... orbit and the stability of the axis (ignoring precession) and show how it causes the seasons; 7.1.5 state the dates of the solstices and equinoxes; 7.1.6 explain the concept of the earth's axial rotation causing day and night; 7.1.7 explain what causes the varying length of daylight through the year ...
