Title: What is Astronomy?
1What is Astronomy?
2Ancient Astronomy
- People have used the stars for ages.
- Used constellations to set planting times
- Used constellations to guide travels
- Some lights in the sky wandered through the
constellations - Called them planets which is Greek for wanderers
3The Mayan Calendar
- The Mayans were the first civilization to widely
use a standard calendar. It consisted of 365
days very much like the calendar we use today.
4Time
- Year Cycle through the seasons as the Earth
revolves around the Sun. - Month Based on cycle of the moon adjusted to
make exactly 12 months in a year instead of the
actual 12.4 cycles per year. - Week 7 is chosen since there are 7 astronomical
objects viewed by Ancient Astronomers besides
the stars Sunday, Moonday, Thorsday (Thor
Jupiter), Saturnday, in English can easily be
identified. In Spanish you can easily identify
Marsday (Martes Tuesday), Mercuryday (Miercoles
Wednesday), and Venusday (Viernes Friday).
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6Time
- Day Time from Noon on one day to Noon on the
next. Noon is the suns highest point. - Hour Day is broken into day and night, and the
daytime is broken into 12 units, just like the
year, and the night is broken into 12 units,
also. Total is 24 hours in a day. - Minute A minute (pronounced my-nute meaning
tiny) part of an hour based on Egyptian idea of
a minute (tiny) part 1/60th . - Second A minute (tiny) part of a minute (tiny)
part of an hour, or a second minute (tiny) part
of an hour, or simply a second.
7Lunar Phases
8Lunar Phases
The moon goes through different phases during the
month because the illuminated (sun-facing) side
changes its orientation relative to the earth.
9Lunar Eclipses
When the moon passes through the Earths shadow,
a lunar eclipse occurs.
10Lunar Eclipses
A total eclipse of the moon.
11Solar Eclipses
Path of a total solar eclipse on the earth.
When the Earth passes through the Moons shadow,
a Solar eclipse occurs.
12Solar Eclipses
A total solar eclipse.
13Tilt of the Earths Axis
- The axis around which the Earth rotates is tilted
by 23.5 degrees with respect to the ecliptic.
14- The seasons are due to the tilt of the Earths
axis. Consider what happens on June 21 when the
northern hemisphere of the Earth is tilted toward
the Sun
Northern Summer
Northern Winter
Southern Summer
Southern Winter
- The sunlight strikes the ground more vertically
than in December. The light is spread out over
less ground and heats the ground better.
15Earth on June 22
16Earth on December 22
17Galileo Galilei (1564-1642)
- He used the telescope to look at astronomical
objects. He discovered craters on the Moon,
moons going around Jupiter, rings around Saturn,
and the fact that Venus has phases that are
related to its orbit. - The heliocentric model can explain all of these,
whereas the geocentric model fails.
18- Tycho Brahe (1546-1601) He collected great
amounts of very precise data about the positions
of the planets using instrumentation he
developed. - Johannes Kepler (1571-1630) He used Brahes data
and mathematics to come up with three laws - Planets follow elliptical instead of circular
orbits. - Planets sweep through equal areas in equal times.
- The square of the period is proportional to the
cube of the semimajor axis of the ellipse.
19Planets
- Move in an elliptical orbit
20Planets
- Period of revolution
- the time it takes to go once around the sun
- One revolution is a year
- Mercury 88 days, Pluto 248 years
21What keeps them there?
- Law of inertia - objects motion wont change
unless acted upon by an outside force. - Wont change speed or direction
- Why do they curve?
- Gravity pulls them toward the sun
22What keeps them there?
23Rotation
- Planets spin on their axes
- One rotation is a day
- Mercury 58 days, Jupiter 10 hours
24A light wave is a light wave, no matter how
long...
25Refracting Telescopes
26Reflecting Telescopes
Refracting telescopes are very similar to
reflecting telescopes, except that the reflecting
telescopes use mirrors, instead of lenses.
27Same Space -- Different Light
Infrared Telescope
Radio Telescope
Optical Telescope
X-ray Telescope
28Light-Year
- To measure distances between stars we a distance
measurement called the Light- year - 1 light-year is the distance light travels in one
year. - Light moves at 300,000 km/sec
- Thats 186,000 mile/sec
- It would reach the sun in about 5 minutes
- How far would it go in a year?
- Nearest star is 4.3 light years away
29Distance to stars
- One method is parallax
- Apparent change in position as the earth goes
around the sun
30Measure the angle to the star
Wait half a year
Measure the angle to the star
Triangle tells distance
31Rockets
- Rely on Netwons Third law of Motion
- For every action there is an equal and opposite
reaction. - Reward blast of hot gases causes rocket to shoot
forward. - First developed by Chinese in 1000
- Tube full of gunpowder with cap on one end.
32Satellites
- If a projectile has a large enough horizontal
(tangential) velocity component (8 km/s), it will
fall around the earth but never strike the
surface. - The result is a circular orbit around the earth.
- For the space shuttle or a satellite to orbit, it
must be above the earths atmosphere to avoid air
resistance (200 km above the surface). - At an altitude of 200 km, the force of the
earths gravity is only slightly reduced.
33Placing the Shuttle into Orbit
- The shuttle is given a vertical thrust from a
rocket to push it up to an altitude of 200 km. - At that point it is given a thrust from another
rocket to increase its tangential speed to 8 km/s.
34Spacecraft
- Probes have gone past all the planets except
Pluto - Have sampled comets tails
- Have taken pictures of planets and moons.