Title: Chapter E Exploring The Heavens
1Chapter EExploring The Heavens
- AST1002 Introduction to Astronomy
- Dr. Mike Reynolds
2What is Astronomy?
- Astronomy, simply stated, is the study of the
Universe. - Astronomers classify objects into numerous groups
- Some of these groupings like stars are easy
to understand scientifically - Others are more difficult
-
3Basic Objects in the Universe
- Stars glowing balls of gas that undergo nuclear
fusion - Planets moderately-large objects orbiting a star
- May be rocky or gaseous
- Visible due to reflecting light
- What is the size to be a planet?
- Usually somewhat spherical, regular-shaped
- Satellite orbits a planet four major groups
- Also called a moon
- Earths satellite Moon (proper noun)
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5Basic Objects in the Universe
- Asteroid relatively small, rocky/metallic object
usually orbiting a star - Comet relatively small, icy object usually
orbiting a star - Solar System Sun and all the objects which orbit
the Sun, including the planets - Star or Stellar System A star and other objects
such as planets and/or other stars and other
materials that orbit it
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7Basic Objects in the Universe
- Moving beyond our Solar System
- Galaxy large island of stars
- Few hundred million to over a trillion stars!
- Galactic Cluster collection of galaxies
gravitationally bound - Supercluster region where galaxies and galactic
clusters are tightly packed - Universe all matter and energy
- Also called the Cosmos
8Some Questions To Ponder
- Can a planet become a star?
- Can a planet be declassified as a planet?
- Can a moon become a planet? Or a planet a moon?
- Does a galaxy have to have stars with planets to
be a galaxy?
9Scale of the Cosmos
- BIG!!!
- Start with Our Solar System
- Earth-Moon distance mean 230,000 miles
- Earth-Sun distance mean 93,000,000 miles
- 1 Astronomical Unit or 1 AU 93,000,000 miles
- The Suns diameter is about 850,000 miles
- The Earths diameter is just under 8,000 miles
- Imagine if the Sun was an Orange
10Motion
- Terms you have heard or will hear
- Rotation the spinning of an object around its
axis - Earth rotates once every 24 hours (approx.)
- Jupiter rotates once every 10 hours (approx.)
- Revolution One object orbiting a second
- Earth revolves around the Sun every 365.24 Earth
Days approx. 1 year - Jupiter revolves around the Sun every 11.86 Earth
Years approx. 1 Jovian year
11The Constellations
- Early peoples told stories about the shapes they
saw in the stars - These shapes are called Constellations
- Today astronomers recognize 88 official
Constellations - Some Constellations are easy to recognize
- Most are not!
- We cannot see all 88 constellations from here we
would need to be at the equator
12Constellations Over the Centuries
- Many peoples identified patterns in the stars
- One example Orion the Hunter, the official
Constellation - China Shen, supreme warrior
- India/Hindus Skanda, celestial general riding a
peacock - Egypt Osiris
- Most of todays 88 official constellations are
Western European in design
13Other Patterns
- Asterism Star pattern within a Constellation
- Not an official Constellation
- The Big and Little Dippers
- within Ursa Major and Ursa Minor
- Pleiades within Taurus
- The Seven Sisters
- Japanese Subaru
- Navajo Dilyehe
- Hawaiian Makahiki or many little eyes
14Our Night Skies
- Celestial Sphere an imaginary sphere on which
all the objects in the sky appear to lie when
observed from a specific place - This sphere appears to surround the Earth
- The Celestial Sphere appears to move
- The Sun and Moon (as well as the bright planets)
also appear on the Celestial Sphere, moving
independently
15Divisions in the Celestial Sphere
- North and South Celestial Poles the points at
which the Celestial Sphere appears to turn/rotate - An extension of Earths axis
- Stars rotate about these points
- Pole Shorthand
- North Celestial Pole NCP
- South Celestial Pole SCP
Polaris
16What Points Do We SeeLooking Up?
- Local Sky sky we see from where we stand
- Ecliptic Suns annual path across the Celestial
Sphere - Why is the Ecliptic not on the Celestial Equator?
- Zenith point directly overhead
- Meridian imaginary line from due north to the
zenith to due south - The Meridian divides the sky into halves
17Other Moving Objects
- The Sun
- Ecliptic path
- Constellations along Ecliptic historically 12
but officially 13 are called the Zodiac - When the Sun is in Leo will the stars
surrounding Leo be visible? - The Moon
- Also travels along the Ecliptic
- Sometimes in the evening sky, sometimes in the
morning, sometimes not visible at all
18Measuring the Sky
How the Sun and Moon Appear to Us in the Sky
- Astronomers use Degrees, Minutes and Seconds to
measure distances across the sky or sizes - Referred to as Angular Sizes the angle the
object appears to span or distance between
objects - Sun and Moon appear to be about ½ degree
- Not their true sizes just how they appear to us
- 60 arcseconds 1 arcminute
- 60 arcminutes 1 degree
½ degree 30 arcminutes
½ degree 30 arcminutes
But in the Real Universe the Sun is 400 times
bigger than the Moon!
19Seasonal Changes
- Seasons occur on a planet or moon because the
axis of rotation remains tilted in one direction
during its orbit - The tilt is relative to the planets or moons
orbit - This tilt results in a planet or moon having
Seasons - Earths axis is tilted about 23 ½ degrees
- Uranus axis is tilted about 98 degrees
Orbital Plane
Earth 23 ½o tilt
Uranus 98o tilt
20Seasons on Earth
- Nothing to do with the distance to the Sun
- Summer in the Northern Hemisphere
- Winter in the Southern Hemisphere
- Winter in the Northern Hemisphere
- Summer in the Southern Hemisphere
- Sun angles in the Summer and Winter make for
differences in temperature -
21Seasonal Terms
- Summer Solstice Suns rays are most-direct
- Winter Solstice Suns rays are least-direct
- Spring or Vernal Equinox Equal day and night,
going from shorter to longer days - Fall or Autumnal Equinox Equal day and night,
going from longer to shorter days
22Some Other Seasonal Stuff
- At the Equinoxes, the Sun rises due east and sets
due west only at the Equinoxes - Noan egg will not stand on end because its the
1st day of Spring (or Fall) - Summer the day is longer, the night shorter
- Extreme at far latitudes midnight Sun
- Winter the day is shorter, the night longer
- Extreme at far latitudes no Sun!
23Will Seasons Always be the Same?
- No! Orientation of Earths axis changes
- Precession the circular motion of a planets
tilted axis - Slow process Earth 26,000 years to complete
one precession - What are the effects of precession?
- Celestial poles change
- Timing of Seasons change
- Nutation A wobble in the wobble!
24The Moon in Our Sky
- It takes 27 1/3 days for the Moon to go around
Earth one time - From new Moon to the next new Moon takes 29 ½
days. - Moonth month!
- Why? Earth has also moved through space and the
Moon has to catch up with that starting position. - Roughly the same side of the Moon faces Earth
- 1 lunar rotation 1 lunar revolution
- One half of the Moon is always illuminated by the
Sun
25The Phases of the Moon
- We see the Moon go through its phases due to the
position of Earth-Moon-Sun relative to each other - NOT
- Clouds
- Moon moves closer or the Sun further away
- Little Green Men aliens
26Moon Phase Terminology
- Crescent Moon less than 50 illuminated
- Gibbous Moon more than 50 but less than 100
- Waxing Growing larger
- New Moon up to Full Moon
- Waning Growing smaller
- Right past Full Moon to New Moon
- Full Moon 100 illuminated
- New Moon 0 illuminated no Moon
27More Moon
- Can you see the Moon in the daytime?
- Yes!
- Does the Moon keep a constant distance from
Earth? - No, varies from a Perigee of about 225,000 miles
to an Apogee of about 243,000 miles - Perigee? Apogee? Refers to the Moons closest and
farthest distances -
28Lunar Eclipses
- A Lunar Eclipse occurs when Earth lies directly
between the Sun and the Moon, so that Earths
shadow falls on the Moon - Three types
- Penumbral
- Partial
- Total
- Entire night side of Earth can see the eclipse
- Total lunar eclipses can vary in color and
brightness due to Earths atmosphere - Red to Copper to Orange to Black!
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32July 1982 Total Lunar Eclipse trail Photograph
by Jay Anderson
33Solar Eclipses
- Four Types
- Partial
- Annular or Ring Eclipse
- Annulars are like a type of partial
- Total
- Total-Annular or Hybrid
- Must be within the eclipse zone to see even a
partial solar eclipse
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36Annular Sequence Photos 10 May 1994
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39Total Solar Eclipses
- Moon totally blocks all harmful solar light and
radiation at totality (not during partial) - Daytime becomes nighttime
- Moons shadow, sunrise/sunset effect
- Animal reactions
- Several events and solar features visible
- Bailys Beads
- Diamond Ring
- Corona
- Prominences
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46Total Solar Eclipses simply the most-spectacular
astronomical event (in my humble opinion)
47Total Solar Eclipses
- Others have been profoundly affected by a total
solar eclipse - St. Benedict
- A total solar eclipse so impacted him that he
started his still-famous work the Benedictine
Society
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