![Earth Science](http://s1.studyres.com/store/data/015663995_1-919bf1ea1c203ef39ff5a8e3f5fe6fd6-300x300.png)
Earth Science
... As with other scientific theories, evidence supports this idea. Besides the red shift of distant stars, there is evidence of cosmic background radiation. This glow, which can be observed all over space, is the leftover energy from the big bang. Working backwards, scientists determine that the big ba ...
... As with other scientific theories, evidence supports this idea. Besides the red shift of distant stars, there is evidence of cosmic background radiation. This glow, which can be observed all over space, is the leftover energy from the big bang. Working backwards, scientists determine that the big ba ...
New Generation Ground-Based Optical/Infrared Telescopes
... solar system. Another recent result was the discovery of comets among the main-belt asteroids. The most recent of these, asteroid 118401 was discovered by the 8-m GeminiNorth telescope. Two other comets in the main belt were detected previously by other astronomers, and many more such comets are now ...
... solar system. Another recent result was the discovery of comets among the main-belt asteroids. The most recent of these, asteroid 118401 was discovered by the 8-m GeminiNorth telescope. Two other comets in the main belt were detected previously by other astronomers, and many more such comets are now ...
time astro 2014 - Fort Thomas Independent Schools
... the caused by the precession of the equinoxes (Earth’s gradual precession causes the orientation of the equatorial plane to shift slightly relative to the ecliptic ...
... the caused by the precession of the equinoxes (Earth’s gradual precession causes the orientation of the equatorial plane to shift slightly relative to the ecliptic ...
Hubble`s Use of Cepheids (PDF version)
... these stars on photographs and had described that to Shapley, when he was still working at Mount Wilson. (Shapley later moved to Harvard.) Shapley had dismissed this as impossible – he ‘knew’ that the spiral nebulae were small, nearby objects. It was galling for him to see Hubble credited with this ...
... these stars on photographs and had described that to Shapley, when he was still working at Mount Wilson. (Shapley later moved to Harvard.) Shapley had dismissed this as impossible – he ‘knew’ that the spiral nebulae were small, nearby objects. It was galling for him to see Hubble credited with this ...
Boonesborough Days - Tri
... had well over 200 visitors stop at our booth each day of the event. Besides having 8 poster displays and 2 computer presentations, we also had 2 telescopes set up for solar viewing along with some solar viewing glasses. As luck would have it, we were fortunate to have one relatively large sunspot an ...
... had well over 200 visitors stop at our booth each day of the event. Besides having 8 poster displays and 2 computer presentations, we also had 2 telescopes set up for solar viewing along with some solar viewing glasses. As luck would have it, we were fortunate to have one relatively large sunspot an ...
Schrödinger`s Equation derived from Newton`s
... The angular velocity of Mercury around the Sun is: θ m' = v m /r m And δ θ’0 = (v m /r m) (180/π) (3600) (26526/Tm); Tm = 88 days And δ θ’0 = 70.75; v m = Mercury orbital velocity around the Sun And v m = 48.1 km/sec; r m = Mercury - Sun distance If Planet Mercury angular speed is measured for plane ...
... The angular velocity of Mercury around the Sun is: θ m' = v m /r m And δ θ’0 = (v m /r m) (180/π) (3600) (26526/Tm); Tm = 88 days And δ θ’0 = 70.75; v m = Mercury orbital velocity around the Sun And v m = 48.1 km/sec; r m = Mercury - Sun distance If Planet Mercury angular speed is measured for plane ...
Lecture16
... distance, we could find their luminosity. We can measure the distance to stars with parallax (our old friend). ...
... distance, we could find their luminosity. We can measure the distance to stars with parallax (our old friend). ...
astronomy history time machine
... Copernicus’s argument that the planets orbit the Sun why the direction of motion of the planets on the celestial sphere sometimes appears to change that Kepler’s determination of the shapes of planetary orbits depended on the careful observations of his mentor, Tycho Brahe how Isaac Newton formulate ...
... Copernicus’s argument that the planets orbit the Sun why the direction of motion of the planets on the celestial sphere sometimes appears to change that Kepler’s determination of the shapes of planetary orbits depended on the careful observations of his mentor, Tycho Brahe how Isaac Newton formulate ...
Big Bang and Life Cycle of Stars
... Then what? The universe expanded very quickly - After a few thousand years, some cooling occurred, which allowed for the formation of atoms – - first Hydrogen and Helium, but it had to cool still more for the other elements to start to form and be neutral atoms -Anti-matter also formed, composed of ...
... Then what? The universe expanded very quickly - After a few thousand years, some cooling occurred, which allowed for the formation of atoms – - first Hydrogen and Helium, but it had to cool still more for the other elements to start to form and be neutral atoms -Anti-matter also formed, composed of ...
Astronomy Exam #2 for the 10
... The hot main sequence stars appear to be mostly B and A spectral type with an absolute magnitude between +2 and -5. This range in absolute magnitudes corresponds to a range in luminosity of between 16 and 10,000 solar luminosities. These stars will have a short main sequence lifetime compared to the ...
... The hot main sequence stars appear to be mostly B and A spectral type with an absolute magnitude between +2 and -5. This range in absolute magnitudes corresponds to a range in luminosity of between 16 and 10,000 solar luminosities. These stars will have a short main sequence lifetime compared to the ...
Working with the Illinois Learning Standards: A Constructivist
... Novas and supernovas are new stars. Stars evolve much as animals evolve. The source of energy of the stars is unknown. As stars shrink due to gravity, they change from red to blue. Red stars are hot; blue stars are cool. Stars are all roughly the same size. Stars change little over their life spans. ...
... Novas and supernovas are new stars. Stars evolve much as animals evolve. The source of energy of the stars is unknown. As stars shrink due to gravity, they change from red to blue. Red stars are hot; blue stars are cool. Stars are all roughly the same size. Stars change little over their life spans. ...
6 - In the Beginning: Science and Genesis 1-11
... “The complete birth of a star has never been observed. The principles of physics demand some special conditions for star formation and also for a long time period. A cloud of hydrogen gas must be compressed to a sufficiently small size so that gravity dominates.” ...
... “The complete birth of a star has never been observed. The principles of physics demand some special conditions for star formation and also for a long time period. A cloud of hydrogen gas must be compressed to a sufficiently small size so that gravity dominates.” ...
Use of Reflected Light with Asteroid Light Curves
... are slight variations from pixel to pixel. These three types of calibration pictures help to eliminate noise. Biases measure the amount of electronic noise inherent in the CCD chip. These do not have an exposure time as it is only measuring electronic noise. Darks measure the thermal noise from runn ...
... are slight variations from pixel to pixel. These three types of calibration pictures help to eliminate noise. Biases measure the amount of electronic noise inherent in the CCD chip. These do not have an exposure time as it is only measuring electronic noise. Darks measure the thermal noise from runn ...
Chapter 30 Notes
... amount of red shift allows astronomers to measure the speed at which these galaxies are moving away. The most distant galaxies are moving away the fastest. Recall the balloon activity where the far away dot moved away at a rate much faster than the two that were close together, when you blew up the ...
... amount of red shift allows astronomers to measure the speed at which these galaxies are moving away. The most distant galaxies are moving away the fastest. Recall the balloon activity where the far away dot moved away at a rate much faster than the two that were close together, when you blew up the ...
Astronomy_Course_Summary
... Students understand the nature of light and its use in astronomy. Target(s) to Meet Learning Objective #4 Discuss the nature of electromagnetic radiation. List the major regions of the electromagnetic spectrum and explain how the properties of Earth's atmosphere affect our ability to make astron ...
... Students understand the nature of light and its use in astronomy. Target(s) to Meet Learning Objective #4 Discuss the nature of electromagnetic radiation. List the major regions of the electromagnetic spectrum and explain how the properties of Earth's atmosphere affect our ability to make astron ...
Spectroscopy pertains to the dispersion of an object`s light into
... beware the high energy UV, x-ray, and gamma-ray photons! Each one carries a lot of energy compared to their visible- and radio-wave brethren. They're the reasons you should wear sunblock, for example. When we look at the Universe in a different "light", i.e. at "non-visible" wavelengths, we probe di ...
... beware the high energy UV, x-ray, and gamma-ray photons! Each one carries a lot of energy compared to their visible- and radio-wave brethren. They're the reasons you should wear sunblock, for example. When we look at the Universe in a different "light", i.e. at "non-visible" wavelengths, we probe di ...
Astrophysics Outline—Option E
... E.3.14 State the relationship between period and absolute magnitude for Cepheid variables E.3.15 Explain hoe Cepheid variables may be used as “standard candles” E.3.16 Determine the distance to a Cepheid variable using the luminosity-period relationship E.4 Cosmology Assessment Statement Olbers’ par ...
... E.3.14 State the relationship between period and absolute magnitude for Cepheid variables E.3.15 Explain hoe Cepheid variables may be used as “standard candles” E.3.16 Determine the distance to a Cepheid variable using the luminosity-period relationship E.4 Cosmology Assessment Statement Olbers’ par ...
Nova
... In Algol-type binaries, one of the stars has evolved and expanded to fill a droplet-shaped potential surface, called the Roche lobe, within which material is gravitationally bound to the star (see Figure 1). The Roche surface is, therefore, the surface along which the gravitational potential is comm ...
... In Algol-type binaries, one of the stars has evolved and expanded to fill a droplet-shaped potential surface, called the Roche lobe, within which material is gravitationally bound to the star (see Figure 1). The Roche surface is, therefore, the surface along which the gravitational potential is comm ...
Photometry - University of Groningen
... • Goal: putting mags on common scale • Standard system= – telescope+filter+detector ...
... • Goal: putting mags on common scale • Standard system= – telescope+filter+detector ...
canopus e.g procyon
... average luminosity of the star. Cepheid variables are also very bright and can be seen from far away. (They are not main sequence stars). A complication though is that there are two populations of Cepheids and they have different period luminosity relations ...
... average luminosity of the star. Cepheid variables are also very bright and can be seen from far away. (They are not main sequence stars). A complication though is that there are two populations of Cepheids and they have different period luminosity relations ...
1 1. The Solar System
... Celestial Sphere: The celestial sphere is an imaginary shell of infinite radius, centered on the observer. This concept is useful for determining positions in the sky. Zenith: This is the point in the sky directly above the observer. Celestial Poles: As the Earth rotates, the sky appears to rotate a ...
... Celestial Sphere: The celestial sphere is an imaginary shell of infinite radius, centered on the observer. This concept is useful for determining positions in the sky. Zenith: This is the point in the sky directly above the observer. Celestial Poles: As the Earth rotates, the sky appears to rotate a ...
CONSTELLATION CANES VENATICI the two hunting dogs Canes
... Supervoid and 1,200 times the volume of expected typical voids. It was discovered in 1988 in a deep-sky survey. • Canes Venatici contains five Messier objects, including four galaxies. The more significant are • the Whirlpool Galaxy (M51, NGC 5194) and NGC 5195, a small barred spiral galaxy that is ...
... Supervoid and 1,200 times the volume of expected typical voids. It was discovered in 1988 in a deep-sky survey. • Canes Venatici contains five Messier objects, including four galaxies. The more significant are • the Whirlpool Galaxy (M51, NGC 5194) and NGC 5195, a small barred spiral galaxy that is ...
Doppler Effect - SAVE MY EXAMS!
... Mark on the wavelength axis the region affected by the atmosphere’s absorption of ultra violet radiation. ...
... Mark on the wavelength axis the region affected by the atmosphere’s absorption of ultra violet radiation. ...
International Ultraviolet Explorer
![](https://en.wikipedia.org/wiki/Special:FilePath/International_Ultraviolet_Explorer.gif?width=300)
The International Ultraviolet Explorer (IUE) was an astronomical observatory satellite primarily designed to take ultraviolet spectra. The satellite was a collaborative project between NASA, the UK Science Research Council and the European Space Agency (ESA). The mission was first proposed in early 1964, by a group of scientists in the United Kingdom, and was launched on January 26, 1978 aboard a NASA Delta rocket. The mission lifetime was initially set for 3 years, but in the end it lasted almost 18 years, with the satellite being shut down in 1996. The switch-off occurred for financial reasons, while the telescope was still functioning at near original efficiency.It was the first space observatory to be operated in real time by astronomers who visited the groundstations in the United States and Europe. Astronomers made over 104,000 observations using the IUE, of objects ranging from solar system bodies to distant quasars. Among the significant scientific results from IUE data were the first large scale studies of stellar winds, accurate measurements of the way interstellar dust absorbs light, and measurements of the supernova SN1987A which showed that it defied stellar evolution theories as they then stood. When the mission ended, it was considered the most successful astronomical satellite ever.