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Star Life Cycle  and classroom textbooks for research!
Star Life Cycle and classroom textbooks for research!

... 2. Find a diagram on the internet showing the life cycle of a star and paste it in your document. (2 pts) 3. Find a “Hertzsprung-Russell Diagram” and paste it in your document. (2pts) 4. Using the diagrams above Answer the following questions. (1 pt each) a. b. c. d. e. f. g. h. i. j. k. l. ...
Week 11 notes
Week 11 notes

... Ionized Hydrogen (HII) • While ionized hydrogen (protons, electrons) forms the majority of the ionized phase of the ISM, it also contains ionized forms of other elements: e.g., OII, OIII, CIV, MgII. • Highest temperature and lowest density of the three gaseous phases (hot, tenuous phase of the ISM): ...
G. Kacprzak "Galaxy-halo and gas connection 0.5 email
G. Kacprzak "Galaxy-halo and gas connection 0.5 email

Topic 9/10
Topic 9/10

... Star- large self-luminous body in space that creates its own energy Nuclear fusion- where the sun gets its energy, 2 hydrogens fuse (combine) to form a helium Sunspots- temporary storms on the visible surface of the sun Galaxy- large body of stars and matter in space, there are over 100 billion gala ...
Solar Lithium Mystery Solved
Solar Lithium Mystery Solved

What is another name for electromagnetic energy?
What is another name for electromagnetic energy?

... List in order the 5 parts of the eye that light hits before sending a signal to the brain. ...
Document
Document

... ● AO imaging and IR spectroscopy of thousands of disks around nearby young stars  diversity of disk systems ● characterize physics of disks T(r), ρ(r) ● detect giant planets directly ● detect giant planets indirectly from gravitational “gaps” in disks ● characterize planets from properties of disk ...
Week 11 Answers
Week 11 Answers

... The more massive stars have shorter lifetimes. Also, the more mass that a main sequence star has, the higher its surface temperature. Cluster D has main sequence stars with surface temperatures all the way up to 20,000 degrees and more. These are stars that do not live for very long as main sequence ...
Learning Targets
Learning Targets

... 15.2 Characteristics of Stars 1. I am able to state the characteristics used for classifying stars. 2. I know how to describe what a light-year is. 3. I know how to use a Hertzsprung-Russell diagram to classify stars. 15.3 Lives of Stars 4. I am able to state the life cycle of small and large stars. ...
Vocabulary Review
Vocabulary Review

... electrons and protons have smashed together to form neutrons ...
Name: Hour:______ Directions for website use: This web activity is
Name: Hour:______ Directions for website use: This web activity is

... Click “Next” (Stellar Personalities): 10. Choose 4 stars from the list and describe their color. (You will need to click “Next” to see their color.) a. ________________________________________________________ b. ________________________________________________________ c. ___________________________ ...
Faintest Star Cluster Yet Found on Outskirts of Milky Way | Globular
Faintest Star Cluster Yet Found on Outskirts of Milky Way | Globular

... which separate light into its constituent wavelengths and allow astronomers to calculate how fast stars are moving, showed that the globular cluster's stars were moving at different velocities than those in Ursa Minor, suggesting the two entities were separate. And very preliminary measurements of t ...
astrocoursespring2012lec2-6
astrocoursespring2012lec2-6

... Stellar classification is a classification of stars based on their spectral characteristics. The spectral classof a star is a designated class of a star describing the ionization of its chromosphere, what atomic excitations are most prominent in the light, giving an objective measure of the temperat ...
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Day-7

... Cassiopeia ...
HR diagram ppt
HR diagram ppt

... 2. Our evidence to support this is ___ ...
Science 8
Science 8

... 5. To measure parallax shift, astronomers look at the same star twice, when Earth is on different sides of the ____________________. ...
When you look up at the night sky, thousands of objects
When you look up at the night sky, thousands of objects

... On the H-R diagram, stars are plotted along the bottom axis by increasing surface temperature, which is measured in units called kelvins (K). (To convert a measurement in kelvins to degrees Celsius, subtract 273 from the kelvin measurement.) Hotter stars are plotted on the left of the diagram, and ...
AST_s309_ss11_2 - University of Texas at Austin
AST_s309_ss11_2 - University of Texas at Austin

... Eliminate Instrumental Shifts Recall that on a spectrograph we only measure a Doppler shift in Dx (pixels). This has to be converted into a wavelength to get the radial velocity shift. Instrumental shifts (shifts of the detector and/or optics) can introduce „Doppler shifts“ larger than the ones due ...
HEIC0619: EMBARGOED UNTIL: 19:30 (CET)/01:30 PM EST 11
HEIC0619: EMBARGOED UNTIL: 19:30 (CET)/01:30 PM EST 11

... or maybe even more – tend to be born in multiple systems that can easily disguise themselves as single very heavy stars. Moreover, these stellar heavyweights are so rare that only a few are close enough to the Sun to be examined in detail. One of the top candidates for the title of “Milky Way stella ...
The Milky Way, Schroedinger`s Cat, and You
The Milky Way, Schroedinger`s Cat, and You

This link is in pdf format for ease of reading
This link is in pdf format for ease of reading

... more complicated structures. Concentrations of matter formed into clouds, then condensed into stars and the collections of stars we call galaxies. The way in which galaxies spin indicates that their visible portions of stars and diffuse gas and dust clouds known as nebulae constitute only one tenth ...
Stellar Evolution
Stellar Evolution

... condense • Temperatures begin to increase = Glows • Fusion begins at VERY high temps. (Some of the extra gas and dust may form planets) ...
Cosmology Unit – FINAL EXAM PRACTICE TEST
Cosmology Unit – FINAL EXAM PRACTICE TEST

... 10. According to the _____ law, a galaxy two times as far away from Earth as a second galaxy will be moving away approximately twice as fast. a. Sagan b. Hubble c. dark matter d. cosmological 11. In the raisin bread analogy for the universe, what do the raisins represent? a. stars b. galaxies c. bl ...
Northam Sky July 2009
Northam Sky July 2009

... What's in the Northam Sky Around mid July just after sunset in Northam if you look due east and about 25 degrees above the horizon you'll see an S shaped collection of stars know as the constellation of Scorpio the scorpion. From the five stars at the top making up Scorpios head and claws through it ...
Electromagnetic Waves Notes
Electromagnetic Waves Notes

... • What do you think exists beyond the red part of the spectrum? • The highest temperature is beyond the red light • There must be some kind of radiation we can’t see! • This unknown radiation is called Infrared Radiation • Before Herschel’s experiment scientists did not know about other types of rad ...
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Astronomical spectroscopy



Astronomical spectroscopy is the study of astronomy using the techniques of spectroscopy to measure the spectrum of electromagnetic radiation, including visible light, which radiates from stars and other hot celestial objects. Spectroscopy can be used to derive many properties of distant stars and galaxies, such as their chemical composition, temperature, density, mass, distance, luminosity, and relative motion using Doppler shift measurements.
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