If the sun and the moon have the same angular diameter on the sky, does that mean that the sun and the moon actually have about the same size?
Yes.
No because the sun is much farther away, but also much larger than the moon.
No, because the sun is much farther away, but also much smaller than the moon.
No because the moon is much farther away, but also much larger than the sun.
No, because the moon is much farther away, but also much smaller than the sun.
Slide 24
Earth’s and Moon’s orbits are slightly elliptical:
Sun
Earth
Moon
(Eccentricities greatly exaggerated!)
Perihelion = position closest to the sun
Aphelion = position furthest away from the sun
Perigee = position closest to Earth
Apogee = position furthest away from Earth
Slide 25
What do you expect to see if at the time of a solar eclipse the moon is near apogee, and the Earth is near perihelion?
A regular total solar eclipse.
No solar eclipse at all.
A partial solar eclipse with a crescent appearance.
A partial solar eclipse with a ring-like appearance of un-occulted parts of the sun.
A lunar eclipse.
Slide 26
Annular Solar Eclipses
The angular sizes of the Moon and the Sun vary, depending on their distance from Earth.
When the Earth is near perihelion, and the Moon is near apogee, we see an annular solar eclipse.
Perigee
Apogee
Perihelion
Aphelion
Slide 27
Almost total, annular eclipse of May 3, 1984
Slide 28
If the moon was orbiting around the Earth exactly in the plane of the ecliptic, …
lunar and solar eclipses would occur once every day.
lunar and solar eclipses would occur once a week.
lunar and solar eclipses would occur once a month.
lunar and solar eclipses would occur once a year.
lunar and solar eclipses would never occur.
Slide 29
Conditions for Eclipses (I)
The Moon’s orbit is inclined against the ecliptic by ~ 5.
A solar eclipse can only occur if the Moon passes a node near New Moon.
A lunar eclipse can only occur if the Moon passes a node near Full Moon.
Slide 3
Conditions for Eclipses (II)
Eclipses occur in a cyclic pattern.
→ Saros cycle: 18 years, 11 days, 8 hours
Slide 31