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Astronomy

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Azimuth = angle E of N from North direction on horizon; ... at vernal equinox and autumnal equinox... rises due E, sets due W, is at 90 - latitude at noon ... – PowerPoint PPT presentation

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Title: Astronomy


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(No Transcript)
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The Altitude Azimuth coordinate system Observer
in Aurora latitude 42º 30 45N
longitude 76º 41 30 W
Altitude angle up from horizon between 0º and
90º
Zenith
Azimuth angle E of N from North direction on
horizon between 0º and 360º
Horizon
3
The Celestial Sphere as seen by an Inuit (living
near the NP)
4
Its Time for Facts about Time
  • Earth rotates steadily, once in 24 h (15º in 1 h)
  • direction is West to East looking down onto
    NP, its counterclockwise (ccw)
  • no matter where you are, local noon is the
    moment
  • exactly halfway between sunrise and sunset
  • when the sun is at its highest point in the sky
  • the sun is due south and therefore is crossing
    the meridian
  • Time zones are a compromise such that the zone
    center, a clock reads 1200 at local noon
  • West of center, local noon occurs up to 30 min
    after 1200 East of center

5
Lets go to the board and talk about degrees and
radians and all that s, q and r language
6
A relationship between sizes
  • D object size ( arc length s) in some units
  • d distance from eye to object ( radius r) in
    same units
  • so subtended angle q angle in radians D/d

To convert q to seconds of angle
  • Since p rad 180º and 1º 60 and 1 60
  • We have q (D/d)(180º/p)(60/º)(60/)
  • So, doing the multiplication we get
  • q 206,265(D/d)
  • where q is in seconds of arc, and D d must be
    in the same length units

7
Insert numbers for a penny d 4 km 4 x 103
m D 2 cm 2 x 10-2 m So q 206,265(D/d)
1.03 x 100 '' 1 ''
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Fig.01.11
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(No Transcript)
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Careful the stars DO NOT MOVE on the celestial
sphere, but the CS rotates once per day We can
see only exactly half of the CS at any moment
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Daily (diurnal) solar motion
  • in one day, the sun barely moves on the celestial
    sphere it just rides along with it.
  • path is never a great circle across the sky
    except
  • at vernal equinox and autumnal equinox
  • rises due E, sets due W, is at 90º - latitude at
    noon
  • day is exactly 12 h long everywhere on Earth
  • in summer, in northern hemisphere
  • Rises north of east (azimuth 90º - latitude)
    and sets north of west (azimuth 270º
    latitude)
  • Day is longer than 12 h
  • Sufficiently far north, sufficiently near summer
    solstice, SUN NEVER SETS!!

12
Looking ahead the Declination-Right Ascension
coordinate system for an observer in North
Canada latitude 75º
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