Homeworks 1: Difference between revisions
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'''Homeworks 1''' is the attempted solution to our second task<ref>Our first task was to register our PRS, visit the course web-page on Blackboard, look at the textbook, and write an equation for our wiki</ref> in the course [[AST4210_5211: Introduction to Astrophysics - Fall 2009|Introduction to Astrophysics]]. This assignment is due on ''Wednesday 09/09/09'' and was assigned on 09/01/09. | '''Homeworks 1''' is the attempted solution to our second task<ref>Our first task was to register our PRS, visit the course web-page on Blackboard, look at the textbook, and write an equation for our wiki</ref> in the course [[AST4210_5211: Introduction to Astrophysics - Fall 2009|Introduction to Astrophysics]]. This assignment is due on ''Wednesday 09/09/09'' and was assigned on 09/01/09. | ||
==Problem 1== | |||
List in order of increasing size and give the approximate size of the following objects: An atom, | |||
a biological cell, a cluster of galaxies, the Earth, a galaxy, the Local Group of galaxies, a neutron, a neutron star, a person, the Solar System, our sun. Note: you may have to look in other books besides your textbook to get all this information. | |||
==Problem 2== | |||
The nearest star outside the solar system is about 4 light years away. | |||
* How far away is the star in kilometers? | |||
* Suppose you travel to the nearest star in a rocket ship moving at 100 km per hour (100 km/hr is | |||
about 62 mi/hr, a typical automobile speed on a Florida highway). How many years will it take | |||
you to get to the star? | |||
* Suppose you travel to the star at 10 km per second (the speed of a rocket in orbit around the | |||
Earth). How many years will it take you to get to the star? | |||
==Problem 3== | |||
Use the size of the Astronomical Unit in kilometers and the length of the year in seconds to calculate how fast the Earth moves in its orbit in kilometers/second. | |||
==Problem 4== | |||
Describe the essential differences between the Ptolemaic, Copernican, and Keplerian descriptions | |||
of planetary motion. | |||
==Problem 5== | |||
Use Newton’s laws to show that the orbits of planets are ellipses. | |||
==References== | ==References== | ||
<references/> | <references/> | ||
Revision as of 19:38, 6 September 2009
Homeworks 1 is the attempted solution to our second task[1] in the course Introduction to Astrophysics. This assignment is due on Wednesday 09/09/09 and was assigned on 09/01/09.
Problem 1
List in order of increasing size and give the approximate size of the following objects: An atom, a biological cell, a cluster of galaxies, the Earth, a galaxy, the Local Group of galaxies, a neutron, a neutron star, a person, the Solar System, our sun. Note: you may have to look in other books besides your textbook to get all this information.
Problem 2
The nearest star outside the solar system is about 4 light years away.
- How far away is the star in kilometers?
- Suppose you travel to the nearest star in a rocket ship moving at 100 km per hour (100 km/hr is
about 62 mi/hr, a typical automobile speed on a Florida highway). How many years will it take you to get to the star?
- Suppose you travel to the star at 10 km per second (the speed of a rocket in orbit around the
Earth). How many years will it take you to get to the star?
Problem 3
Use the size of the Astronomical Unit in kilometers and the length of the year in seconds to calculate how fast the Earth moves in its orbit in kilometers/second.
Problem 4
Describe the essential differences between the Ptolemaic, Copernican, and Keplerian descriptions of planetary motion.
Problem 5
Use Newton’s laws to show that the orbits of planets are ellipses.
References
- ↑ Our first task was to register our PRS, visit the course web-page on Blackboard, look at the textbook, and write an equation for our wiki