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ASTR 1102-002 2008 Fall Semester. Joel E. Tohline, Alumni Professor Office: 247 Nicholson Hall [Slides from Lecture02]. Course Syllabus ( corrected Final Exam time!). Evaluation of Coursework. Corrected final exam time!. Chapter 17: The Nature of Stars. Describe Population (of stars).
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ASTR 1102-0022008 Fall Semester Joel E. Tohline, Alumni Professor Office: 247 Nicholson Hall [Slides from Lecture02]
Evaluation of Coursework Corrected final exam time!
Describe Population (of stars) • Location • Coordinate position • Distance • Motion • Across the photo/sky • Toward/away from us • Intrinsic properties • Mass • Color • Brightness • Age
Describe Population (of fans) • Location • Coordinate position • Distance • Motion • Across the photo/sky • Toward/away from us • Intrinsic properties • Mass (weight) • Color (clothes) • Brightness (?) • Age
Location – Determine exact location of every fan! • Coordinate position • Distance
Location – Determine exact location of every fan! • Coordinate position (x-y coordinate on photo) • Distance (distance from photographic lens)
Location – Determine exact location of every fan • Coordinate position (x-y coordinate on photo) straightforward • Distance (distance from photographic lens)
Location – Determine exact location of every fan • Coordinate position (x-y coordinate on photo) • Distance (distance from photographic lens) not so straightforward!
e.g., Google Earth • Location – or … using GPS system … • Coordinate position (latitude & longitude) • Distance (altitude above sea level)
Location – Determine exact location of every star! • Coordinate position • Distance
Location – Determine exact location of every star! • Coordinate position (“declination” & “right ascension”) • Distance (from Earth)
Straightforward: Analogous to “latitude” & “longitude”; e.g., Google Sky Textbook ‘Box 2-1’ pp. 30-31 • Location – Determine exact location of every star! • Coordinate position (“declination” & “right ascension”) • Distance (from Earth)
Location – Determine exact location of every star! • Coordinate position (“declination” & “right ascension”) • Distance (from Earth) not so straightforward!
Determining Distances to Astronomical Objects • Not at all straightforward! • Only direct method is “Stellar Parallax” • See textbook discussion associated with Figs. 17-1 and 17-2 • Other indirect methods will be discussed later
Individual Stars… • Location in Space • Coordinate (angular) position on the sky • Distance from Earth • Motion through Space • Motion across the sky (“proper” motion) • Motion toward/away from us (radial velocity) • Intrinsic properties • Brightness (luminosity/magnitude) • Color (surface temperature) • Mass • Age
Individual Stars… • Location in Space • Coordinate (angular) position on the sky • Distance from Earth • Motion through Space • Motion across the sky (“proper” motion) • Motion toward/away from us (radial velocity) • Intrinsic properties • Brightness (luminosity/magnitude) • Color (surface temperature) • Mass • Age
Motion • Across the photo/sky • Toward/away from us • Location • Coordinate position • Distance
Motion • Across the photo/sky • Toward/away from us • Location • Coordinate position • Distance
Motion • Across the photo/sky • Toward/away from us • Location • Coordinate position • Distance
Motion Across the Sky(“proper” motion) http://www.psi.edu/~esquerdo/jim/astfov.gif
Motion • Across the photo/sky • Toward/away from us • Location • Coordinate position • Distance
Determining Motion of Astronomical Objects toward/away • Surprisingly straightforward! • Doppler effect • See textbook discussion in Chapter 5, §5-9
Doppler Effect (§5-9) • The measured frequency (wavelength) of light changes if the light source is moving toward or away from you • Light is “blue-shifted” if the object is moving toward you • Light is “red-shifted” if the object is moving away from you • Direct analogy with the behavior of sound waves
Individual Stars… • Location in Space • Coordinate (angular) position on the sky • Distance from Earth • Motion through Space • Motion across the sky (“proper” motion) • Motion toward/away from us (radial velocity) • Intrinsic properties • Brightness (luminosity/magnitude) • Color (surface temperature) • Mass • Age
Individual Stars… • Location in Space • Coordinate (angular) position on the sky • Distance from Earth • Motion through Space • Motion across the sky (“proper” motion) • Motion toward/away from us (radial velocity) • Intrinsic properties • Brightness (luminosity/magnitude) • Color (surface temperature) • Mass • Age