Motions in the Sky - University of Wisconsin–Stevens Point
Transcript of Motions in the Sky - University of Wisconsin–Stevens Point
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Lecture 2
Motions in the Sky
September 10, 2018
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What is your year in school?
A. New freshman
B. Returning freshman
C. Sophomore
D. Junior
E. Senior
F. I’ve been here, like,
forever
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What is your major?3
A. Arts or Communication
B. Natural Resources
C. Professional Studies
D. One of the Sciences
E. One of the Humanities (languages,
philosophy, political science, etc.)
F. Undeclared
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Why are you taking this class?
A. Astronomy seems interesting to
me.
B. Only because it satisfies my
GEP requirements.
C. It was the only class that would
fit in my schedule.
D. A friend recommended it to me.
E. Some other reason.
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Units of Measure
• We’ll use mainly the metric system, based on the
meter, kilogram, and second
• We’ll often use scientific notation:
• You should know the metric prefixes and
scientific notation
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1 light-year 9,461,000,000,000,000 m
9.461 10 m
=
=
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Angular Size
• Astronomers measure angles in degrees and
arc minutes (60 per degree) and arc seconds
(60 per arc minute)
• The size of an object is related to its
distance from Earth and its observed
angular diameter
physical diameter distance angular diameter 180
57.3
rD
=
=
D
r
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Estimating Angles
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Jupiter has a physical diameter of 143,000 km
and is 635,000,000 km from Earth. What is
its angular size?
A. 46.5 arcsec
B. 129 arcsec
C. 635 arcsec
D. 1910 arcsec
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Jupiter has a physical diameter of 143,000 km
and is 635,000,000 km from Earth. What is
its angular size?
A. 46.5 arcsec
B. 129 arcsec
C. 635 arcsec
D. 1910 arcsec
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( )5
8
57.357.3
57.3
57.3 1.43 10 km0.0129
6.35 10 km
3600 arcsec0.0129 46.5 arcsec
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r DD D r
r
= = =
= =
= =
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Yearly Motions
• The Earth travels around the Sun once every
year.
• The Earth is tilted by 23.5 degrees with
respect to the orbital plane.
E
E
E
E
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• The Sun lines up with different constellations
during the year.
These stars are overhead during the
day. Sun is too bright to see them.
These stars are visible at night.
Presently
These stars are visible at
night.
These stars are overhead during the
day. Sun is too bright to see them
6 months later
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What is a Day?
• Solar Day = amount of time for Earth
to rotate once on its axis with respect
to the Sun.
• Sidereal day = amount of time for
Earth to rotate once with respect to
the stars.
– Shorter than solar day by 4 minutes.
• Since solar and sidereal days are
NOT the same, a star will typically
rise 4 minutes earlier each day.
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Ecliptic
• Path of the sun
through the
celestial sphere.
• Not aligned
with Celestial
Equator due to
tilt of the Earth
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Zodiac• The 13 constellations through which the sun
passes during the course of a year.
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Interactive Figure (might not work in every browser)
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Constellation Traditional Actual (2000) Days
Capricornus Dec. 22-Jan. 21 Jan. 21-Feb. 16 26
Aquarius Jan. 22-Feb. 21 Feb. 16-Mar. 11 24
Pisces Feb. 22-Mar. 21 Mar. 11-Apr. 18 38
Aries Mar. 22-Apr. 21 Apr. 18-May 13 25
Taurus Apr. 22-May 21 May 13-June 22 40
Gemini May 22-June 21 June 22-July 21 29
Cancer June 22-July 21 July 21-Aug. 10 20
Leo July 22-Aug. 21 Aug. 10-Sept. 16 37
Virgo Aug. 22-Sept. 21 Sept. 16-Oct. 31 45
Libra Sept. 22-Oct. 21 Oct. 31-Nov. 23 23
Scorpius Oct. 22-Nov. 21 Nov. 23-Nov. 29 6
Ophiuchus Nov. 29-Dec. 18 19
Sagittarius Nov. 22-Dec. 21 Dec. 18-Jan. 21 34
The Real Signs of the Zodiac15
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If we could observe background stars in daylight,
how would the Sun appear to move against this
background because of the Earth’s orbit around the
Sun?
A. 1° per day, from west to east
B. 1° per day, from east to west
C. 15° per hour, from west to east
D. 15° per hour, from east to west
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Planetary Motion
The planets all move in
the same plane about the
Sun so they all appear to
move along the zodiac
(near the ecliptic).
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Summer Solstice North Celestial Pole
South Celestial PoleCelestial Equator
Ecliptic
Summer Solstice:Sun reaches highest point
in sky for N. Hemisphere.
(June 21)Longest period of
daylight in Northern
Hemisphere
E
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Autumnal EquinoxEqual periods of day and night for entire Earth
E
North Celestial Pole
South Celestial PoleCelestial Equator
Ecliptic
Autumnal Equinox:Sun crosses Celestial
Equator. (September 21)
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Winter Solstice
Longest period of
darkness in Northern
Hemisphere
North Celestial Pole
South Celestial PoleCelestial Equator
Ecliptic
Winter Solstice:Sun at lowest point in
sky for N. Hemisphere.
(December 21)
E
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Vernal EquinoxEqual periods of day and night for entire Earth
North Celestial Pole
South Celestial PoleCelestial Equator
Ecliptic
Vernal Equinox:Sun crosses Celestial
Equator. (March 21)
E
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The ecliptic crosses the celestial equator at ___
A. Two points, known as solstices
B. Two points, known as equinoxes
C. One point, known as the vernal
equinox
D. One point, known as the meridian
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The Seasons• The Seasons are due to the tilt of the Earth
with respect to the orbital plane.
– Not distance from sun
• Flash Applet
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Why are the seasons warm and cold?• During the Summer the sun is higher in the sky
so the light is more direct.
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• Sun is above the horizon longer in the
summer.
Why are the seasons warm and cold?
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During summer in the northern hemisphere, why is
it still cold at the North Pole, even though they get
24 hours of daylight?
A. The Earth is further from the
Sun in the summer.
B. The North Pole is further from
the Sun than Stevens Point
C. The light is still very indirect
even in the summer.
D. None of the above.
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