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Quiz about Lost Outdoors Just Look to the Sky
Quiz about Lost Outdoors Just Look to the Sky

Lost Outdoors? Just Look to the Sky! Quiz


If you ever get lost while hiking or camping, navigating and telling time using the heavens can be a critical survival skill. Here are a few methods to estimate time and direction, valid in the Northern Hemisphere, below 50° latitude.

A multiple-choice quiz by mcdubb. Estimated time: 8 mins.
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Author
mcdubb
Time
8 mins
Type
Multiple Choice
Quiz #
306,129
Updated
Dec 03 21
# Qns
10
Difficulty
Difficult
Avg Score
4 / 10
Plays
1038
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Question 1 of 10
1. The easiest way to find direction at night in the Northern Hemisphere is to find Polaris, the North Star, since it always points due north. Besides finding north, what other critical information can be indicated by the angle of Polaris between the observer, the star, and the horizon? Hint


Question 2 of 10
2. During the day when the North Star is not visible, the Sun can be used to find direction. In the Northern Hemisphere, what direction is the Sun when it is at its highest point in the sky? Hint


Question 3 of 10
3. A common belief is that the Sun always rises due east, and sets due west. This is true for the equinoxes, however the further away you are from the vernal or autumnal equinox, the differences in location for sunrise and sunset increase. In June in the Northern Hemisphere, from what direction does the Sun rise? Hint


Question 4 of 10
4. When using the Sun, Moon, and stars to tell time, it is important to know the difference between solar and local time. The definition of solar noon is the time when the Sun is at its highest point in the sky. This time is approximately 12:00 pm, but a few factors can contribute to solar and local noon differing by up to an hour or two. When converting solar noon to the actual local time, which of the following factors in the least? Hint


Question 5 of 10
5. If lost in the wild, knowing the time to sunset can play an important role when deciding when to start preparing a shelter for the night. One method of estimating the time until sunset is the "four fingers" method. This method entails holding out your arm, and tilting your hand sideways, palm facing you. Line up the bottom of your little finger (digitus minimus) with the horizon below the Sun. Each finger width between the top of the Sun and the horizon represents fifteen-minute increments until sunset, and four fingers is an hour. If it is the afternoon, the Sun is "six fingers" above the horizon using the "four fingers" method, and sunset is around 6:00 pm, what is the approximate time? Hint


Question 6 of 10
6. If lost without a clock, the Moon can be a fantastic tool used to approximate the time of day. The phase of the moon can be used to indicate where the Sun is in relation to the Earth and Moon, and hence the solar time. For instance, a full moon is always highest in the sky at solar midnight, when the sun is directly behind the observer. By the same logic, a new moon is always highest in the sky at solar noon, although not visible. Halfway between a full moon and a new moon, a third quarter moon is highest at 6:00 am. Using this information, if the Moon is a waning gibbous and it is at its highest point in the southern sky, what is the approximate solar time? Hint


Question 7 of 10
7. If the Moon is a waxing crescent, and it is in its highest point in the southern sky, what is the approximate solar time? Hint


Question 8 of 10
8. The time the Moon takes to traverse the sky is dependent on its phase and time of year. If an observer is in a place where a day is 10 hours long in the winter and 14 hours long in the summer, a first quarter moon will be visible for 10 hours in the fall, and 14 hours in the spring. A first quarter moon is always highest in the sky at 6:00 pm solar time. If it is springtime for this observer, and a first quarter moon is eight finger widths above the eastern horizon using the "four fingers" method, what is the current solar time? Hint


Question 9 of 10
9. Since the Earth makes one rotation per day, the stars in the northern sky appear to make one rotation about the North Star each day. This can be a handy tool used to tell time, but it involves a bit of math using the "Big Dipper Clock." In the "Big Dipper Clock," imagine an inverted 24-hour clock centered around the North Star, moving counter-clockwise. For this clock, the normal 3:00 position is 6:00 pm, 12:00 is midnight, and the normal 9:00 position is 6:00 am. Every 30 degrees, an hour on a normal clock, represents two hours on the Big Dipper Clock. The "hour hand" in this case is the imaginary line drawn from the North Star to the two stars that make up the far edge of the "bowl" of the Big Dipper (Alpha Ursae Majoris and Beta Ursae Majoris). To account for the Earth's revolution around the Sun, add two hours for every month after March 7, or four minutes per day, and this is the current solar time. For example, if the "hour hand" is in the 2:00 position, that represents 8:00 pm on the "Big Dipper Clock." On March 7, it would be 8:00 pm and on May 7, it would be midnight solar time. If the hour hand of the Big Dipper Clock is facing the normal 11:00 position on April 7, what is the approximate solar time? Hint


Question 10 of 10
10. If the hour hand of the "Big Dipper Clock" is at a 45 degree angle between 9:00 and 12:00 on a normal clock, or the 10:30 position, and it is January 7th, what is the local solar time? Hint



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Quiz Answer Key and Fun Facts
1. The easiest way to find direction at night in the Northern Hemisphere is to find Polaris, the North Star, since it always points due north. Besides finding north, what other critical information can be indicated by the angle of Polaris between the observer, the star, and the horizon?

Answer: Latitude

The angle of Polaris above the horizon is always equal to the observer's latitude. If Polaris is at a 45° angle, then the observer is at 45° latitude. If Polaris is at a 30° angle, then the observer is standing at 30° latitude.
2. During the day when the North Star is not visible, the Sun can be used to find direction. In the Northern Hemisphere, what direction is the Sun when it is at its highest point in the sky?

Answer: South

The Sun traverses across the sky from east to west, and it at its highest point while due south in the Northern Hemisphere. To best estimate when the Sun is at its highest point, find a location with a clear view of the southern sky, and plant a stick in the ground.

In the dirt, trace the path of the end of the stick's shadow. After noon, the line between the shortest point between the line traced and the stick points due south.
3. A common belief is that the Sun always rises due east, and sets due west. This is true for the equinoxes, however the further away you are from the vernal or autumnal equinox, the differences in location for sunrise and sunset increase. In June in the Northern Hemisphere, from what direction does the Sun rise?

Answer: Northeast

The higher latitude for an observer, the greater the difference from due east and west the sun rises and sets per time of year. When the day is longer in the summer, the Sun takes longer to traverse the sky. The longest path is from northeast in the morning, south at noon, and northwest at sunset. The shortest path, in the winter, is from southeast to south to southwest.
4. When using the Sun, Moon, and stars to tell time, it is important to know the difference between solar and local time. The definition of solar noon is the time when the Sun is at its highest point in the sky. This time is approximately 12:00 pm, but a few factors can contribute to solar and local noon differing by up to an hour or two. When converting solar noon to the actual local time, which of the following factors in the least?

Answer: Distance of the Moon from the Earth

If an observer is on the edge of two time zones, the difference between solar noon and local noon can differ by a half hour or more. Local time for an observer in the center of their time zone is usually the closest to solar time. If the observer is in Daylight Saving Time as well, depending on time of year the difference is an additional hour. If the Earth were divided up evenly into 24 segments, each segment would be 15° in width.

However, time zones tend to follow geopolitical boundaries rather than exact longitude, contributing to additional error. Also, solar time can vary by up to 18 minutes depending on the time of year due to the eccentricity of Earth's orbit.

However, local time for most observers would never be off from solar time by more than a half hour outside of Daylight Saving Time.

The distance of the Moon from the Earth, depending on the location if the Moon's orbit, may perturb Earth's orbit slightly and hence solar time, but this effect is insignificant.
5. If lost in the wild, knowing the time to sunset can play an important role when deciding when to start preparing a shelter for the night. One method of estimating the time until sunset is the "four fingers" method. This method entails holding out your arm, and tilting your hand sideways, palm facing you. Line up the bottom of your little finger (digitus minimus) with the horizon below the Sun. Each finger width between the top of the Sun and the horizon represents fifteen-minute increments until sunset, and four fingers is an hour. If it is the afternoon, the Sun is "six fingers" above the horizon using the "four fingers" method, and sunset is around 6:00 pm, what is the approximate time?

Answer: 4:30 pm

This estimation works best when sunset is within two to three hours or so, or eight to twelve finger widths above the horizon. It can also be used to estimate the amount of time that has passed since sunrise. Of course, there are exceptions if the observer has abnormally sized fingers!
6. If lost without a clock, the Moon can be a fantastic tool used to approximate the time of day. The phase of the moon can be used to indicate where the Sun is in relation to the Earth and Moon, and hence the solar time. For instance, a full moon is always highest in the sky at solar midnight, when the sun is directly behind the observer. By the same logic, a new moon is always highest in the sky at solar noon, although not visible. Halfway between a full moon and a new moon, a third quarter moon is highest at 6:00 am. Using this information, if the Moon is a waning gibbous and it is at its highest point in the southern sky, what is the approximate solar time?

Answer: 3:00 am

If the Moon is a waning gibbous, one quarter of the way between full and new, it will rise about three hours after sunset, and set three hours after sunrise. This is about 9:00 pm to 9:00 am at the equinoxes and equator, and will vary by season and latitude. Each of the eight lunar phases is at its peak in the southern sky (in the Northern Hemisphere, northern sky for Southern Hemisphere) in 3 hour intervals.

A full moon is at its peak at midnight, waning gibbous at 3:00 am, third quarter at 6:00 am, waning crescent at 9:00 am, new moon at 12:00 pm, waxing crescent at 3:00 pm, first quarter at 6:00 pm, and waxing gibbous at 9:00 pm.
7. If the Moon is a waxing crescent, and it is in its highest point in the southern sky, what is the approximate solar time?

Answer: 3:00 pm

If the Moon is a waxing crescent, one quarter of the way between a new moon and a full moon, it will rise about three hours after sunrise, and set three hours after sunset. This is about 9:00 am to 9:00 pm at the equinoxes and equator, and will vary by season and latitude.
8. The time the Moon takes to traverse the sky is dependent on its phase and time of year. If an observer is in a place where a day is 10 hours long in the winter and 14 hours long in the summer, a first quarter moon will be visible for 10 hours in the fall, and 14 hours in the spring. A first quarter moon is always highest in the sky at 6:00 pm solar time. If it is springtime for this observer, and a first quarter moon is eight finger widths above the eastern horizon using the "four fingers" method, what is the current solar time?

Answer: 1:00 pm

If the length of a day vs. date were plotted on a graph over the course of a year, it forms a sine wave, with a peak in the summer and a valley in the winter. A first quarter moon is physically at a 90° angle facing left, between the Earth and Sun. If plotted against the length of day, the time it takes a first quarter moon to traverse the sky is a sine wave shifted 90° to the left, or three months, meaning it is visible for the longest time in the spring, and shortest in the fall. A third quarter moon's path is shifted 90° to the right, meaning it is visible the longest in the fall, and shortest in the spring. A new moon follows the path of the Sun, so its traverse is equal to the length of day. It is offset 0° from the Sun and Earth, and so is its chart. A full moon is at a 180° angle between the Earth and Sun, so its chart is offset 180°, or six months. A full moon is visible for the longest in the winter, and shortest in the summer since it always rises at sunset, and sets at sunrise.

For this example, since it is springtime, the first quarter moon is visible for 14 hours. A first quarter moon is highest at 6:00 pm, meaning it must have risen 7 hours earlier, at 11:00 am. Using the "four fingers" method, since it is eight finger widths above the horizon, or two hours later, the time is 1:00 pm.
9. Since the Earth makes one rotation per day, the stars in the northern sky appear to make one rotation about the North Star each day. This can be a handy tool used to tell time, but it involves a bit of math using the "Big Dipper Clock." In the "Big Dipper Clock," imagine an inverted 24-hour clock centered around the North Star, moving counter-clockwise. For this clock, the normal 3:00 position is 6:00 pm, 12:00 is midnight, and the normal 9:00 position is 6:00 am. Every 30 degrees, an hour on a normal clock, represents two hours on the Big Dipper Clock. The "hour hand" in this case is the imaginary line drawn from the North Star to the two stars that make up the far edge of the "bowl" of the Big Dipper (Alpha Ursae Majoris and Beta Ursae Majoris). To account for the Earth's revolution around the Sun, add two hours for every month after March 7, or four minutes per day, and this is the current solar time. For example, if the "hour hand" is in the 2:00 position, that represents 8:00 pm on the "Big Dipper Clock." On March 7, it would be 8:00 pm and on May 7, it would be midnight solar time. If the hour hand of the Big Dipper Clock is facing the normal 11:00 position on April 7, what is the approximate solar time?

Answer: 4:00 am

The 11:00 pm position on the normal clock, one hour before midnight on a normal clock, means that it is two hours after midnight on an inverted 24-hour clock, or 2:00 am, since the hour hand travels counter clockwise. Add two hours for every month after March 7. Since for this example it is April 7, the current solar time is 4:00 am.
10. If the hour hand of the "Big Dipper Clock" is at a 45 degree angle between 9:00 and 12:00 on a normal clock, or the 10:30 position, and it is January 7th, what is the local solar time?

Answer: 11:00 pm

If the hour hand is at 10:30 on the normal clock, a 45 degree angle or halfway between midnight and 6:00 am, then the inverted 24 hour clock of "Big Dipper Clock" is indicating 3:00 am. Since the date is January 7, two months prior to March 7, subtract 4 hours. This indicates that the solar time is approximately 11:00 pm.
Source: Author mcdubb

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