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Transcript
Survey of the Universe
Tom Burbine
[email protected]
All stars rotate around Polaris throughout the evening
http://www.flickr.com/photos/odalaigh/1482685365/
Polaris
• Polaris' altitude, or height above the horizon, is
equal to an observer's latitude.
http://www.geographyalltheway.com/ks3_geography/maps_atlases/longitude_latitude.htm
Celestial Coordinates
• Coordinates on the celestial sphere
• Right ascension – east-west position (hours, minutes,
seconds)
• Declination – north-south position (degrees)
http://www.oneminuteastronomer.com/3924/sky-coordinates/
Zodiac
• The zodiac is an imaginary belt in the heavens
extending approximately 8 degrees on either side
of the Sun's apparent path (the ecliptic), that
includes the apparent paths of the Moon and the
planets Mercury, Venus, Mars, Jupiter, Saturn,
Uranus, and Neptune.
Question:
• Why do all the planets seem to
follow the same path?
Answer:
• The planets, the Earth, and the Sun
all tend to fall in the same plane
called the ecliptic
Celestial Equator
• Extension of the Earth’s equator into the Celestial
Sphere
Question:
• Why is the path of the constellations
on the zodiac not on the celestial
equator?
Answer:
• The rotation axis of the Earth is
inclined with respect to the ecliptic
Long Term Changes
Precession
• Earth precesses like a top
• Precession - phenomenon by which the axis of a
spinning object (e.g. a part of a gyroscope)
"wobbles" when a torque is applied to it
Forces
• For a top, the force is gravity, which is trying to
pull the top down
• For the Earth, the forces are due to the pull of the
Sun and Moon, which is trying to align the
Earth’s axis with the ecliptic
Because of precession
• The position of a star that corresponds to the
North Celestial Pole changes
What causes seasons?
• The tilt of the Earth’s axis relative to the ecliptic
Seasons
Solstices
• Summer Solstice –June 21 – Northern
Hemisphere receives its most direct sunlight
• Winter Solstice – December 21 – Northern
Hemisphere receives its least direct sunlight
Equinoxes
• Sun shines equally on both hemispheres
• Spring Equinox – March 21 – Northern
Hemisphere goes from slightly tipped away from
the Sun to slightly tipped towards
• Fall Equinox – September 21 - Northern
Hemisphere goes from slightly tipped toward
from the Sun to slightly tipped away
Why does the orbital
difference not matter?
Reasons
• There is only a 3% difference in the distance from
the Earth to the Sun at its farthest and closest
point
• The Earth is actually closer to the Sun in the
winter than in the summer
Seasons
• Everybody should watch this video on why we
have seasons
• http://www.learner.org/resources/series28.html?p
op=yes&pid=9#
Any Questions?