ASTR-1010 Planetary Astronomy

Slides:



Advertisements
Similar presentations
Chapter 6: Telescopes – Portals of Discovery. Visible light is only one type of electromagnetic radiation emitted by stars Each type of EM radiation travels.
Advertisements

Electromagnetic Radiation and Telescopes
Chapter 6: The Tools of the Astronomer
Astronomy and the Electromagnetic Spectrum
The EM Spectrum & Earth September 30, 2009.
Chapter 6 Optics and Telescopes
Chapter 6 Telescopes: Portals of Discovery. 6.1 Eyes and Cameras: Everyday Light Sensors Our goals for learning How does your eye form an image? How do.
Astronomy 1010 Planetary Astronomy Fall_2014 Day-22.
X-Ray UltravioletVisibleInfraredRadio The Electromagnetic Spectrum and the Universe.
Optics and Telescopes Chapter 5 Survey of Astronomy om astro1010-lee.com.
Chapter 21 Stars, Galaxies, and the Universe.  How do we study other stars in our galaxy if they are so far away?  We study the radiation that stars.
1 Earth’s Atmosphere & Telescopes Whether light is absorbed by the atmosphere or not depends greatly on its wavelength. Earth’s atmosphere can absorb certain.
Light and Telescopes Chapter 5. Traditional Telescopes The 4-m Mayall Telescope at Kitt Peak National Observatory (Arizona)
Chapter 3: Telescopes. Goals Describe basic types of optical telescopes Explain why bigger is better for telescopes Describe how the Earth’s atmosphere.
Collecting and Mapping Planetary Data. Direct measurements (in situ) Collecting data directly at the site of scientific interest Ground stations on Earth.
Telescopes (Chapter 6). Based on Chapter 6 This material will be useful for understanding Chapters 7 and 10 on “Our planetary system” and “Jovian planet.
January 24, 2006Astronomy Chapter 5 Astronomical Instruments How do we learn about objects too far away for spacecraft? How do telescopes work? Do.
Question 1 Modern telescopes use mirrors rather than lenses for all of these reasons EXCEPT 1) Light passing through lenses can be absorbed or scattered.
Studying space from Earth Tele = distance Scopos = to watch Light and radiation How astronomers gather info about space.
Light and Telescopes What do you think? What is the main purpose of a telescope? Why do stars twinkle?
Objective: I will relate the electromagnetic spectrum to wavelengths of light energy. 9/30/14.
Space Technology Telescopes Chapter 18 Section 2.
Telescopes Chapter 5. Objectives   Telescopes……………Chapter 5 Objectives:   1. To list the parts of a telescope.   2. To describe how mirrors aid.
Telescopes & Light: Part 1. A Telescopes is a tool used to gather light from objects in the universe.
Chapter 6: The Tools of the Astronomer. Telescopes come in two general types Refractors use lenses to bend the light to a focus Reflectors use mirrors.
Modern Telescopes Lecture 12. Imaging Astronomy in 19c Photography in 19c revolutionize the astronomy Photography in 19c revolutionize the astronomy 
Chapter 3 Light and Telescopes. What do you think? What is the main purpose of a telescope? Why do stars twinkle?
ASTR-1010 Planetary Astronomy Day Announcements Smartworks Chapters 4: Due Monday, March 1. Smartworks Chapter 5 is also posted Exam 2 will cover.
Light and Telescopes.
Light and Telescopes.
Astronomy and the Electromagnetic Spectrum
© 2010 Pearson Education, Inc. Chapter 6 Telescopes: Portals of Discovery.
Optics and Telescopes. Optics and Telescopes: Guiding Questions 1.How do reflecting and refracting telescopes work? 2.Why is it important that professional.
© 2004 Pearson Education Inc., publishing as Addison-Wesley Telescopes.
How do colors in a spectrum help us understand stars? Image from
Astronomical Tools. Essential Questions 1.What is Light? 2.How do telescopes work, and how are they limited? 3.What kind of instruments do astronomers.
ASTR-1010 Planetary Astronomy Day HOMEWORK Homework Chapter 2: Due Today Motions of the Sun Motions of the Sun – Due Today Exam -1 – Next time–
Tools of Modern Astronomy Chapter 21 Section 1 Pages Chapter 21 Section 1 Pages
Chapter 6 Telescopes: Portals of Discovery. 6.1 Eyes and Cameras: Everyday Light Sensors Our goals for learning How does your eye form an image? How do.
The Origin and Nature of Light. Honors Project Deadlines Sorry about the confusion!! Project Proposal Deadline: Thursday March 1 st 2007 Project Submission.
Optics and Telescopes Chapter Six. Introducing Astronomy (chap. 1-6) Introduction To Modern Astronomy I Ch1: Astronomy and the Universe Ch2: Knowing the.
Clicker Questions Chapter 3 Telescopes Copyright © 2010 Pearson Education, Inc.
Exploring Space – Course 3
Section 1 – pg 590 Telescopes
The Origin and Nature of Light
1 Stellar Astronomy Spring_2015 Day-18.
Telescopes. Light Hitting a Telescope Mirror huge mirror near a star * * * small mirror far from 2 stars In the second case (reality), light rays from.
Astronomy 1020 Stellar Astronomy Spring_2015 Day-22.
Astronomy 1010-H Planetary Astronomy Fall_2015 Day-17.
ASTR-1010 Planetary Astronomy Day Announcements Homework Chapter 3: Due Wednesday Feb. 24 Smartworks Chapters 4 & 5 are also posted Exam 2 will.
What Channel is That?.  Visible light is a form of electromagnetic radiation.  Others include:  Radio waves  Infrared waves (heat)  Ultraviolet waves.
Astronomy 1010-H Planetary Astronomy Fall_2015 Day-23.
Astronomy 1010-H Planetary Astronomy Fall_2015 Day-24.
Chapter 21: Stars, Galaxies, Universe Section 1: telescopes
Astronomy 1010 Planetary Astronomy Fall_2015 Day-23.
Tools of Astronomy Chapter 28.1 Pages The Best Tool The Light that comes to earth from distant objects is the best tool that astronomers can.
Astronomy 1010 Planetary Astronomy Fall_2015 Day-17.
The Very Large Array (VLA) in New Mexico. Observations at wavelengths other than visible light are revealing previously invisible sights Visible light.
Universe Tenth Edition Chapter 6 Optics and Telescopes Roger Freedman Robert Geller William Kaufmann III.
Astronomy 1010 Planetary Astronomy Fall_2015 Day-24.
Telescopes. Light Hitting a Telescope Mirror huge mirror near a star * * small mirror far from a star In the second case (reality), light rays from any.
Astronomy 1020 Stellar Astronomy Spring_2016 Day-19.
Chapter 6 Telescopes: Portals of Discovery
Homework #4 What is the maximum resolution of your eyes (assume the wavelength range that your eyes are sensitive to is 300 – 700 nm and that your iris.
Tuesday September 8, 2015 Agenda
© 2017 Pearson Education, Inc.
Telescopes.
Light and Telescopes
Light and Telescopes.
Review When is Orion visible in Arizona?
Presentation transcript:

ASTR-1010 Planetary Astronomy Day - 19

Announcements Smartworks Chapters 4: Due Monday, March 1. Smartworks Chapter 5 is also posted Exam 2 will cover chapters 3, 4, & 5 -Target Wednesday, March 3 ***Bring your Lecture-Tutorial books to the exam. They will be collected and graded. - Make SURE your name is in it!

Once a site with good “seeing” is found everyone wants to use it Kitt Peak, AZ

Mauna Kea Hawaii

Today most observations are done with a CCD Camera

CCD’s are much more sensitive than photographic film

ClassAction Stuff CCD Simulator Splash page questions

If you pass white light through a prism, it separates into its component colors. long wavelengths ROY G B I V short wavelengths spectrum

Another common measuring device is the spectrograph

The best spectrographs use diffraction gratings

The spectrograph/CCD produces a black & white spectrum

Spectra can be displayed as a graph or rainbow of color

Multitasking Saves Time

But visible light is only one type of electromagnetic radiation (light) emitted by stars Astronomers are truly interested in the entire spectrum of Light!

Consider This Class as Seen in Different Wavelengths of Light!

Consider Orion as Seen in Different Wavelengths of Light!

Observations at other wavelengths are revealing previously invisible sights UV infrared Map of Orion region Ordinary visible

Radio wavelength observations are possible from Earth’s surface

Observing In Radiowaves Long Wavelength…poor resolution

Under the dish at Arecibo

The Very Large Array (VLA)

Saturn In Different Wavelengths Near IR Visible Radio

Astronomers use different instruments to look at light of different wavelengths - sometimes, we even have to go above Earth’s atmosphere.

Not all EM radiation can penetrate Earth’s atmosphere.

Atmospheric Windows

Telescopes and Earth’s Atmosphere Lecture Tutorial pg. 49 Work with a partner! Read the instructions and questions carefully. Discuss the concepts and your answers with one another. Take time to understand it now!!!! Come to a consensus answer you both agree on and write complete thoughts into your LT. If you get stuck or are not sure of your answer, ask another group.

Which is the correct reasoning for why a gamma ray telescope located in Antarctica that is to be used to look for evidence of black holes in the centers of galaxies would not get funded? There is no way to detect the presence of a black hole. Gamma rays are too energetic to detect with a telescope. You can’t build a functioning telescope in Antarctica. Gamma rays don’t penetrate Earth’s atmosphere.

Imagine you’re the head of a funding agency that can afford to build only one telescope. Which of the four proposed telescopes below would be best to support? A gamma ray telescope in Antarctica A radio telescope in orbit above the Earth A visible telescope located high on a mountain in Peru An ultraviolet telescope located in the Mojave desert