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Astronomy 1 — Elementary Astronomy LA Mission College
Spring F2015
Light and Telescopes
Astronomy 1 - Elementary Astronomy LA Mission College Levine F2015
Quotes & Cartoon of the Day
“We find them smaller and fainter, in constantly increasing numbers, and we know that we are reaching into space, farther and farther, until, with the faintest nebulae that can be detected with the greatest telescopes, we arrive at the frontier of the known universe.”
Edwin Powell Hubble
Astronomy 1 - Elementary Astronomy LA Mission College Levine F2015
Announcements
• HW Kepler, Gravity Light posted
• Due 10/15
• CoC Star Party Friday
Star Party
Join us for a
Friday,
OCT 16
7 – 9:30 p.m.Carl A Rasmussen AmphitheaterCollege of the Canyons Canyon Country Campus17200 Sierra Highway, Santa Clarita, CA 91351
COLLEGE OF THE CANYONS • Canyon Country Campus
STAR FORMATION: Light Beyond The VisiblePresented by Dr. Luisa RebullResearch Scientist, SSC and IRSA, IPAC, CaltechFeaturing: • Hands-on interactive demonstrations and activities
• COC student clubs and academic departments highlighting innovative approaches to understanding the science that governs the universe
• Gaze at the stars through a variety of telescopes
Food and beverages will be available for purchaseFor more information visit
www.canyons.edu/ccc • COL
LEGE OF THE CANYONS •
CANYON COUNTRY
Tallest TowerBuilding CompetitionSign-up online!
www.canyons.edu/Offices/CCC/Pages/StarParty.aspx
Astronomy 1 - Elementary Astronomy LA Mission College Levine F2015
Last Class
• LT EM Spectrum
• Telescopes & Observatories
• Light and the Atmosphere
• Multi-wavelength Astronomy
Astronomy 1 - Elementary Astronomy LA Mission College Levine F2015
This Class
• Midterm debrief
• Multi-wavelength Astronomy
• Intro to the Solar System
Astronomy 1 — Elementary Astronomy LA Mission College
Spring F2015
Multiwavelength Astronomy
Astronomy 1 - Elementary Astronomy LA Mission College Levine F2015
Astronomers observe across the Electro-magnetic spectrum
• Gamma rays
• X-rays
• the ultraviolet (UV)
• visible light
• the infrared (IR)
• submillimeter & radio
WHAT WE LEARN ABOUT AT DIFFERENT WAVELENGTHS
Astronomy 1 - Elementary Astronomy LA Mission College Levine F2015
Infrared: More than Your Eyes Can See
Astronomy 1 - Elementary Astronomy LA Mission College Levine F2015
Xray & Gamma Ray Astronomy
• Hot objects & violent events
• matter heated to millions of degrees
• cosmic explosions, high speed collisions, material moving at extremely high speeds.
• Black Holes
• Supernovae
• White dwarfs & pulsars
• Hottest part of Sun’s atmosphere
• observatories must be in space
Compton Gamma Ray Observatory
Image Credit: NASA
Astronomy 1 - Elementary Astronomy LA Mission College Levine F2015
Infrared Astronomy
• Old, cold & dusty objects
• space based observatories or high-flying aircraft.
• A few narrow bands from Earth
• heat radiation from cool objects
• penetrate thick interstellar dust
• star-forming regions
• central areas of our galaxy
• Cool stars
• cold interstellar clouds
• star-forming galaxies
• planets
Spitzer Space TelescopeNASA/JPL-Caltech/R. Hurt (SSC)
Astronomy 1 - Elementary Astronomy LA Mission College Levine F2015
Radio ( & Microwave) Astronomy
• Very cold objects, traces atomic and molecular hydrogen
• Radiation left over from the Big Bang
• supernovae
• quasars
• interstellar gas and molecules
Very Large Array (VLA)
Image courtesy of NRAO/AUI
Astronomy 1 — Elementary Astronomy LA Mission College
Spring F2015
The Solar System
Astronomy 1 - Elementary Astronomy LA Mission College Levine F2015
Key Properties of the Solar System
• Disk shape (mostly)
• Orbits lie nearly in a plane
• Dominant common direction of rotation & revolution
Astronomy 1 - Elementary Astronomy LA Mission College Levine F2015
Key Properties of the Solar System
• 2 types of planets
• Terrestrial/Rocky • Dense, inner SS
• Mercury, Venus, Earth, Mars
Astronomy 1 - Elementary Astronomy LA Mission College Levine F2015
Key Properties of the Solar System
• 2 types of planets
• Jovian/Gas Giant
• Low density, outer SS
• planetary rings, many satellites
• Jupiter, Saturn, Uranus, Neptune
Astronomy 1 - Elementary Astronomy LA Mission College Levine F2015
Key Properties of the Solar System
• Lots of small bodies
• “debris”
• moons, dwarf planets, asteroids, comets, meteoroids, kuiper belt objects
Asteroid 243 Ida & DactylAugust 28, 1993
Image Credit: NASA
Astronomy 1 - Elementary Astronomy LA Mission College Levine F2015
Key Properties of the Solar System
• Lots of empty space
• Common age ~4.6 billion years
Astronomy 1 - Elementary Astronomy LA Mission College Levine F2015
Lots of Empty Space
Asteroid belt in movies
Astronomy 1 - Elementary Astronomy LA Mission College Levine F2015
Lots of Empty Space
Asteroid belt “real life”
1 km asteroid~1 in
next nearest asteroid to scale is 15 miles away
Astronomy 1 - Elementary Astronomy LA Mission College Levine F2015
Neil DeGrasse Tyson on Killer Asteroids
SOLAR SYSTEM SCALE & STRUCTURE
Astronomy 1 - Elementary Astronomy LA Mission College Levine F2015
Contents & Scale of the Solar System
• Unit of distance for SS is Astronomical Unit or AU
• 1 AU is distance Earth-Sun
• 1 AU = about 150 million kilometers, or 93 million miles
• Overview of Contents
• The Sun
• Inner SS & Terrestrial planets & Asteroid Belt (0-~5 AU)
• Outer SS & Jovian Planets (~5-30 AU)
• Kuiper Belt (30-50 AU)
• Heliopause (~230 AU)
• Voyager spacecraft!!!!!!
• Oort Cloud (hypothetical) (50,000-100,000 AU)
Astronomy 1 - Elementary Astronomy LA Mission College Levine F2015
Anatomy of the Solar System 0-5 AU
• The Sun
• Inner SS
• Mercury
• Venus
• Earth/Moon
• Mars
• Asteroid belt, between the orbits of Mars and Jupiter
http://www.cosmosportal.org
Astronomy 1 - Elementary Astronomy LA Mission College Levine F2015
Anatomy of the Solar System
• The Sun
• Inner SS
• Outer SS (5-30 AU)
• Jupiter
• Saturn
• Uranus
• Neptune
Astronomy 1 - Elementary Astronomy LA Mission College Levine F2015
Anatomy of the Solar System
• The Sun
• Inner SS
• Outer SS
• Kuiper Belt/Kuiper-belt objects (KBOs)
• 30-50 AU
• Pluto & other dwarf planets
Astronomy 1 - Elementary Astronomy LA Mission College Levine F2015
Anatomy of the Solar System
• Heliopause • Termination shock can be considered edge of SS
• Voyager spacecraft now interstellar!
• Launched in 1977
Astronomy 1 - Elementary Astronomy LA Mission College Levine F2015
Video Voyager Goes Interstellar
http://www.space.com/22752-voyager-1-goes-interstellar-solar-system-boundary-passed-video.html#ooid=l5OGF5cDp4DTaZp2mYwJDkkYCM-
UV7I4
Astronomy 1 - Elementary Astronomy LA Mission College Levine F2015
Anatomy of the Solar System
• Oort Cloud (hypothetical)
http://abyss.uoregon.edu
LET’S PRACTICE
Astronomy 1 - Elementary Astronomy LA Mission College Levine F2015
Rank the following in order of increasing radius: I. The Sun II. Jupiter’s orbit around the Sun III. Earth’s orbit around the Sun IV. The Heliopause
A. I, II, III, IV
B. IV, II, III, I
C. I, III, II, IV
D. I, IV, III, II
Astronomy 1 - Elementary Astronomy LA Mission College Levine F2015
Most of the space in the solar system is filled by
A. the Sun
B. the terrestrial planets
C. the Jovian planets
D. empty space
WARM-UP QUESTION
Astronomy 1 - Elementary Astronomy LA Mission College Levine F2015
The Sun has a diameter of approximately 1.4 million kilometers. Roughly how many Earths would fit across the diameter of the Sun?
A. 10
B. 100
C. 1000
D. 10,000
E. 1 million
LT SUN SIZE
Astronomy 1 - Elementary Astronomy LA Mission College Levine F2015
The Sun has a diameter of approximately 1.4 million kilometers. Roughly how many Earths would fit across the diameter of the Sun?
A. 10
B. 100
C. 1000
D. 10,000
E. 1 million
Let’s Practice
Astronomy 1 - Elementary Astronomy LA Mission College Levine F2015
The image at right shows a picture of the Sun. The dark spots located on this image are sunspots. How does the size of Earth compare to the size of the sunspot that is identified on the right side of the image of Sun?
A. Earth and the sunspot are about the same size.
B. The sunspot is much, much larger than Earth.
C. The sunspot is much, much smaller than Earth.
Sun Size – Instructor’s Guide 129
© 2013 Pearson Higher Education, Inc. Instructor’s Guide for Lecture-Tutorials for Introductory Astronomy
Third Edition
diameter by that of the Moon. Here is an opportunity to talk about proportional reasoning skills.
9) [ 220 orbital diameters ]
Since 110 Sun diameters would fit between Earth and the Sun and 2 orbital diameters of the Moon would fit across the Sun, then 220 Moon orbital diameters would fit between the Sun and Earth.
ADDITIONAL QUESTIONS 1) The image at right shows a picture of the Sun. The dark spots located on this image are
sunspots. How does the size of Earth compare to the size of the sunspot that is identified on the right side of the image of Sun?
a) Earth and the sunspot are about the
same size. b) The sunspot is much, much larger than
Earth. c) The sunspot is much, much smaller than
Earth.
2) Which statement do you think best represents the size comparison between the diameter of the Sun and the distance between the Moon and Earth? The Sun’s diameter is a) smaller than the distance between the Moon and Earth. b) approximately equal to the distance between the Moon and Earth. c) larger than the distance between the Moon and Earth.
3) If you were constructing a scale model of the solar system that used a Sun that was the size of a basketball (approximately 12 inches in diameter), which of the following lengths would most closely approximate the scaled distance between Earth and the Sun? a) 3 feet (length of an outstretched arm) b) 10 feet (height of a basketball goal) c) 100 feet (height of an 10 story building) d) 300 feet (length of a football field)
Astronomy 1 - Elementary Astronomy LA Mission College Levine F2015
Which statement do you think best represents the size comparison between the diameter of the Sun and the distance between the Moon and Earth? The Sun’s diameter is
A. smaller than the distance between the Moon and Earth.
B. approximately equal to the distance between the Moon and Earth.
C. larger than the distance between the Moon and Earth.
Astronomy 1 - Elementary Astronomy LA Mission College Levine F2015
If you were to construct a scale model of the solar system that used a 2 cm cherry to represent the Moon, how large of a ball would you need to represent the Sun?
A. 4cm
B. 30cm
C. 110 cm
D. 440 cm
E. 880 cm
WRAP-UP
Astronomy 1 - Elementary Astronomy LA Mission College Levine F2015
Topic for Next Class
• Sun, Earth & Moon
Astronomy 1 - Elementary Astronomy LA Mission College Levine F2015
Reading Assignment
• Astro: 5&7
• Astropedia: 5 & 11
Astronomy 1 - Elementary Astronomy LA Mission College Levine F2015
Homework
• Kepler, Gravity & Light due 10/15