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Astro 10 Practice Test 2
Astro 10 Practice Test 2

... 1. Each giant molecular cloud is likely to form only one star when the cloud collapses. 2. The key to measuring the masses of stars is to observe and measure the mutual orbits of eclipsing binary stars. 3. One of the important `ingredients’ for the Sun’s magnetic field is the fact that there’s a lay ...
Improving the Gaia planet catch by combining the astrometry with
Improving the Gaia planet catch by combining the astrometry with

Answer - OKBU.net
Answer - OKBU.net

New light on our Sun`s fate - Space Telescope Science Institute
New light on our Sun`s fate - Space Telescope Science Institute

... employ multi-object spectrographs on large 10-meter class telescopes, such as the Keck telescopes in Hawaii, to measure spectra for dozens of white dwarfs in a given cluster at one time. We then compare computer models of those hydrogen lines with a white dwarf’s spectrum to measure its surface pres ...
Excellence
Excellence

... the H/ R diagram you can tell that white dwarfs are not very bright (10 – 10, 000 x dimmer than our sun) and they are of spectral type O, B, A, F. So white dwarfs are smaller, more dense, and much dimmer than red giants. They are hotter than red giants and are in different spectral classes (OBAF) as ...
Star Show FACILITATOR NOTES
Star Show FACILITATOR NOTES

... including both continuous and line characteristics.) Emphasize the temperature-color link by pointing out that an incandescent light bulb which closely matches the Sun’s spectrum must have a temperature very close to the temperature at the Sun’s visible surface—well over 5000°C. Except for specializ ...
Characteristics of Stars (Ph)
Characteristics of Stars (Ph)

... called giant stars or supergiant stars. If the supergiant star Betelgeuse (bay tul jooz) were located where our sun is, it would be large enough to fill the solar system as far out as Jupiter. Some stars are much smaller than the sun. White dwarf stars are about the size of Earth. Neutron stars are ...
Beyond Our Solar System
Beyond Our Solar System

... In this figure, your field of view widens by a factor of 100, and you can see an area 1 mile in diameter. – The arrow points to the scene shown in the preceding photo. – People, trees, and sidewalks have vanished, but now you can see a college campus and the surrounding streets and houses. – The di ...
Apparent Magnitude
Apparent Magnitude

Archaeologists Say the `Anthropocene` Is Here—But It Began Long
Archaeologists Say the `Anthropocene` Is Here—But It Began Long

... smaller exoplanets—down to Earth-size a more promising 9 months for the system’s 62f, falls outside the strictly defined habitand below—and more and more exoplanets outermost known planet, called Kepler-62f. able zone but inside a more loosely defined that are in the habitable zone, where a solid, Alt ...
Starry Monday at Otterbein
Starry Monday at Otterbein

... Galileo’s Genius – Applied to Sunspots • Careful observation of a phenomenon – Observes sunspots (as did others before him) – Follows them over several weeks ...
WORD - hrsbstaff.ednet.ns.ca
WORD - hrsbstaff.ednet.ns.ca

... the type of star, size of star, and the star’s stage of evolution. (d) It plots a star’s size and surface temperature, which allows astronomers determine its region of origin. 49. What is the Main Sequence? (a) The evolutionary path, as seen on the H-R diagram, that a star follows throughout its lif ...
File
File

... within a molecular cloud caused by nearby supernovas or other forces.  Most stars spend about 90% of their life-times as main sequence stars. During this time hydrogen is turned into helium by nuclear fusion at the star’s core. As the main sequence stage continues the luminosity, temperature and he ...
Homework #7 (Ch. 19)
Homework #7 (Ch. 19)

... Low mass stars evolve at a slower rate than high mass ones; this principle applies equally to the process of formations. If a star cluster forms any O or B stars, they will use up their hydrogen and die out before many of the lowest mass stars have time to evolve onto the main sequence. The powerful ...
Star`s ReadingStar`s Reading(es)
Star`s ReadingStar`s Reading(es)

... Since galaxies are so far apart, most of the universe is empty space. If our galaxy were the size of a dime, the Andromeda Galaxy would be about half a meter away. The rest of the universe, as far as astronomers can see, would extend for about 2 kilometers in all directions. Distances to Stars Dista ...
Star Formation
Star Formation

... Convection Zone ...
d Transparent Deception In yet Another Alleged Extra
d Transparent Deception In yet Another Alleged Extra

... announced the discovery of a fifth planet around the star 55 Cancri, which is 41 light years away in the constellation Cancer. The find makes that star system the most heavily populated one known other than our sun's and raises to 265 the total of extra solar planets since astronomers began discover ...
Stars - PAMS-Doyle
Stars - PAMS-Doyle

... Motion of Stars • They rotate on an axis • They may revolve around another star • They move toward or away from our solar system. • The Doppler Effect can determine their direction…works just like sound in the apparent shift because of motion! ...
ph709-08-3b - Centre for Astrophysics and Planetary Science
ph709-08-3b - Centre for Astrophysics and Planetary Science

... is smaller than those from earlier studies but is consistent within measurement errors and also with theoretical estimates of the radii of irradiated Jupiter-like planets. Satellites or rings orbiting the planet would, if large enough, be apparent from distortions of the light curve or from irregula ...
SPECIAL REPORT
SPECIAL REPORT

... metal-poor stars. This is commonly taken as proof of core accretion’s dominance: Metal-rich stars presumably had metal-rich ...
presentation source
presentation source

... “[Even though T Tauri associations could all have similar colors implying young age by coincidence], it is of course, tempting to search for a connection between the T Tauri stars and Bok’s ‘globules,’ but we must admit that at present there is no evidence of any objects intermediate between the two ...
Characteristics of Stars - Laconia School District
Characteristics of Stars - Laconia School District

Orbits of the planets - University of Iowa Astrophysics
Orbits of the planets - University of Iowa Astrophysics

3 Exam #1
3 Exam #1

... 35. For each of the terrestrial planets (plus the Moon), compare the relative size of the core. 36. What two factors determine whether or not a planet will be able to retain an atmosphere? Explain how they compete with each other. 37. For each of the processes mentioned (cratering, volcanism, tecton ...
NAME:______ANSWER KEY_______________________Period
NAME:______ANSWER KEY_______________________Period

... 2. What does light year measure? distance 3. Why do we use light year instead of kilometers? Kilometers would be way to big of a number 4. Change the following number 78,000,000 to scientific notation. 7.8 x 107 5. Write 1.90 x 108 in standard number form. 190,000,000 6. Define Nebula: a large cloud ...
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