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The NakedEye Observatory at MTSU

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Identify the North Star by mapping northern constellations with respect to time. ... Interpret circumpolar constellations in terms of a spherical Earth. ... – PowerPoint PPT presentation

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Title: The NakedEye Observatory at MTSU


1
The Naked-Eye Observatory at MTSU
2
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  • 70 foot by 70 foot square
  • Sun is 32 feet in diameter
  • The Sun will have scale sunspots and prominences

4
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5
Observatory Plan
  • Larger circle is 40 feet in diameter.
  • 16 foot diameter dome.

6
Observatory Elevation
7
Observatory Elevation
  • Top of dome is 18 feet high
  • Base of dome is 12 feet high

8
Typical Column Front
9
Typical Column Back
10
Column Elevation
  • Columns are 10 feet tall.
  • Markers are 3 to 5 feet tall.

11
  • Sun
  • Mercury
  • Venus
  • Earth
  • Mars
  • Asteroid Belt
  • Jupiter
  • Saturn
  • Uranus
  • Neptune
  • Pluto/Kuiper Belt
  • Entire Solar System or Comets

12
The Jupiter (North) Column
  • Each column has a scaled image of a solar system
    object.
  • Each column has factoids inscribed.
  • Each column has a symbol on the outside to
    attract attention.

13
North and South Grids
14
East and West Grids
15
Planetary Symbols
16
Potential Experiments
  • Identify the North Star by mapping northern
    constellations with respect to time.
  • Determine the latitude of Murfreesboro.
  • Learn basic principles of celestial navigation.

17
Potential Experiments
  • Identify circumpolar constellations.
  • Use these constellations to tell time.
  • Interpret circumpolar constellations in terms of
    a spherical Earth.

18
Potential Experiments
  • Examine sunrise and sunset points to explain the
    Earths tilt and the seasons.
  • Identify the first days of Spring, Summer, Fall,
    and Winter.
  • Examine the moonrise and moonset times/elongation
    angles to explain lunar phases.
  • Identify the paths of the planets through the sky.

19
Potential Experiments
  • Identify where and when to look in the night sky
    for meteor showers.
  • Calculate angular size of Sun and Moon and
    relative distances to Sun and Moon.

20
Potential Experiments
  • Measure Earths rotation rate.
  • Measure Earths rate of revolution around the Sun.

21
Potential Experiments
  • Calculate local noon from Suns shadow.
  • Compare local noon with Central Time to explain
    time zones.
  • Find true north using the Suns shadow.
  • Understand why it is different from magnetic
    north.

22
Potential Experiments
  • Measure altitude of Sun at local noon throughout
    the year.
  • Use latitude of Murfreesboro and solar altitudes
    to measure solar declination.
  • Estimate the time from the Suns shadow.
  • Estimate the date from the Suns shadow.

23
Potential Experiments
  • Measure distance to Mars via elongation angles.
  • Measure Earths diameter from the angles of
    shadows.
  • Practical exercises in spherical trigonometry
  • Predict when the Moon will be at a node/eclipse
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