Exploring the Universe I The Solar System Homework Assignment 3
Exploring the Universe I The Solar System Homework Assignment 3
Exploring the Universe I The Solar System Homework Assignment 3
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Name:<br />
Student No:<br />
Astronomy 310 – <strong>Exploring</strong> <strong>the</strong> <strong>Universe</strong> I<br />
<strong>The</strong> <strong>Solar</strong> <strong>System</strong><br />
<strong>Homework</strong> <strong>Assignment</strong> 3<br />
Due by: 2:00 p.m., Thursday, May 31, 2007 in <strong>the</strong> slot outside Henn 312<br />
1. Telescope Funding (adapted from Adams, Pra<strong>the</strong>r and Slater (2005) “Lecture Tutorials for Introductory<br />
Astronomy”)<br />
Recall that Earth’s atmosphere blocks, or partially blocks,<br />
some wavelengths of light (as shown in <strong>the</strong> diagram.) This<br />
is important information to telescope designers. It is also<br />
important to funding agencies who decide which projects<br />
to fund after considering <strong>the</strong> following:<br />
• certain wavelengths of light are blocked from reaching<br />
Earth’s surface by <strong>the</strong> atmosphere<br />
• <strong>the</strong> proposed location for <strong>the</strong> telescope<br />
• telescopes in space are much more expensive to construct<br />
than Earth-based telescopes.<br />
Based on <strong>the</strong>se criteria, for each pair of proposals below,<br />
decide which one should receive funding and explain why<br />
you made that decision.<br />
this is <strong>the</strong> diagram<br />
from <strong>the</strong> in-class worksheet<br />
“Telescopes and Earth’s Atmosphere”<br />
(a) Project Bart: an x-ray telescope, located near <strong>the</strong> North Pole, used to examine <strong>the</strong> Sun<br />
Project Lisa: an infrared telescope, in orbit around <strong>the</strong> Earth, used to view <strong>the</strong> formation of nearby<br />
solar systems<br />
(b) Project Jordan: a large, optical telescope built in <strong>the</strong> Rockies in British Columbia<br />
Project Blake: a small, optical telescope on <strong>the</strong> outside of <strong>the</strong> International Space Station<br />
Astronomy 310 (Newbury) Summer 2007
2. Roving Mars Scientists controlling <strong>the</strong> $700 million Mars Rover Spirit do not want to drive it off a cliff!<br />
Every command must be confirmed before it is carried out, just in case <strong>the</strong> message is corrupted on <strong>the</strong> way<br />
to Mars. With <strong>the</strong> current time-delay of 17 minutes, this makes controlling Spirit a slow process.<br />
Imagine <strong>the</strong> following simple task. Spirit has identified an interesting rock 10 metres away. Your job is to<br />
drive <strong>the</strong> rover over to <strong>the</strong> rock, activate <strong>the</strong> camera, take a picture and transmit <strong>the</strong> picture back to Earth.<br />
Assume it takes 30 minutes for <strong>the</strong> rover to roll to <strong>the</strong> rock but all o<strong>the</strong>r activities take no time to complete.<br />
Complete <strong>the</strong> following log entry, recording <strong>the</strong> commands you send (JPL), Spirit’s transmissions (S), <strong>the</strong><br />
time it takes (T) for <strong>the</strong> command to reach <strong>the</strong> recipient and <strong>the</strong> total elapsed time (TET) for <strong>the</strong> mission.<br />
<strong>The</strong> beginning of <strong>the</strong> conversation is given. (Add ano<strong>the</strong>r page if you need more space.)<br />
# Communication T TET<br />
(min) (H:M)<br />
1. JPL: Drive forward 10 metres 17 0:17<br />
2. S: Please confirm, “drive forward 10 metres” 17 0:34<br />
3. JPL: Confirm: drive forward 10 metres 17 0:51<br />
4. S: drives 10 metres 30 1:29<br />
5.<br />
Astronomy 310 (Newbury) Summer 2007