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Doppler Effect Demo
Doppler Effect Demo

... that are close to the Milky Way actually move toward us and are blue-shifted. However, all galaxies beyond a certain distance are red-shifted. Is it possible to see any planets orbiting other stars? As of the time of this writing (August 2002) no planets have been directly observed. Most extra-solar ...
Project 2. CCD Photometry
Project 2. CCD Photometry

... Standard stars are required so that different observers are able to compare results  with each other. The reason this is true is because every observational setup is likely  to have different response functions, so the same stars will not be observed to have  the  same  brightness  (even  relative  ...
Introduction to Astronomy (high school)
Introduction to Astronomy (high school)

Setting the Stage for Habitable Planets
Setting the Stage for Habitable Planets

... radiation (particles and short wavelength electromagnetic radiation) can damage the ozone UV shield on a planet with an oxygen-rich atmosphere [14]. In the Solar System, the solar wind modulates the cosmic ray flux (from beyond the Solar System) and affects their flux at the Earth [15]. There is som ...
How Big is the Solar System?
How Big is the Solar System?

... walked up till then). This gap marks the boundary between the inner and outer solar systems. The inner solar system contains the four small, hard, "terrestrial" (Earth-like) planet; the outer solar system contains the four large, fluid, "Jovian" (Jupiter-like) planets, with the exception of Pluto. I ...
HR DIAGRAM (Page 1) - McDonald Observatory
HR DIAGRAM (Page 1) - McDonald Observatory

... expands the photosphere of the star, puffing it up and changing the effective temperature. As a result, the star “leaves” the main sequence as it evolves. This phase of a star’s life is called the “giant phase”. In this phase, the core temperature and luminosity of the star has increased, but the ef ...
Star Maps and Constellations (pdf 3.7 Megs)
Star Maps and Constellations (pdf 3.7 Megs)

... Herschel showed that the eye does not respond to brightness linearly, i.e. it does not perceive an object twice as bright to be twice as bright. Instead, an object which is 100 times brighter is perceived to be only 5 magnitudes brighter. The formal relationship between (perceived) magnitude differe ...
Spectroscopic Data
Spectroscopic Data

Star Formation in Our Galaxy - Wiley-VCH
Star Formation in Our Galaxy - Wiley-VCH

... Along with their gas, molecular clouds contain an admixture of small solid particles, the interstellar dust grains. These particles efficiently absorb light with wavelengths smaller than their diameters (about 0.1 µm) and reradiate this energy into the infrared. Regions where the dust effectively bl ...
PLANETS
PLANETS

PDF format
PDF format

... Why do photographs of a star field show some stars to be larger than others? ...
Here
Here

... After the Main Sequence: Low Mass • The core collapses until the gas is “degenerate”, at which point it acts like a solid. It becomes a white dwarf: – The density is more than 1 million times that of water. – The source of support is the “electron degeneracy” pressure. The maximum mass that can be ...
Great Migrations & other natural history tales
Great Migrations & other natural history tales

Searching for Baby Planets in a Star`s Dusty Rings
Searching for Baby Planets in a Star`s Dusty Rings

... linked to the condensation or evaporation of dust grains that occur at different distances from the star because of large radial temperature gradients in the disk. Alternatively, they could arise from the concentration of millimeter-sized particles in regions of gas where the turbulence is low or th ...
Constraints on the exosphere of CoRoT-7b*
Constraints on the exosphere of CoRoT-7b*

... plasma torus of Io, we select these lines for our study. Figure 1 shows the coadded spectrum of CoRoT-7b of data-set I. The wavelength is in the rest frame of the star. The full line is the spectrum taken in-transit, and the dashed line is the spectrum taken out-of-transit. The S/N of the coadded sp ...
key - Scioly.org
key - Scioly.org

... 64. Globular clusters primarily consist of what population stars? [1] 65. Do OoI or OoII clusters have higher metallicity? [1] 66. As globular clusters age, what stars tend to drift inward? [1] 67. What was the first known globular cluster? [1] 68. What is the largest globular cluster in the Milky W ...
Astrophysics notes - School
Astrophysics notes - School

... Magnitude is a measure of how bright a star is. There are, however, two different ways of indicating a stars magnitude; apparent magnitude and absolute magnitude. The scale we use to measure magnitude is based on that created by the ancient Greeks which ran from 1 to 6. On the ancient Greek scale 1 ...
Motions of the Stars
Motions of the Stars

... In reality, the stars are in constant motion. Great distances make the amount of motion small on a human lifetime. ...
Spring 2017 - Astronomers of Humboldt
Spring 2017 - Astronomers of Humboldt

... Jupiter is at opposition on April 7 and the planet rises at sunset; however, due to the glare of the setting sun, Jupiter is best seen after twilight. For April and May, Jupiter will be out all night so it is possible to view the planet from mid-evening to dawn. The opposition of Jupiter is the star ...
Document
Document

... societies, it is warfare. In each case, a strong force was required to achieve the resulting integration. The parallel becomes clearer when we examine more closely the corresponding fusion processes involved. How fast the conversion of hydrogen into helium takes place within a star depends not only ...
Deep Space Mystery Note Form 3
Deep Space Mystery Note Form 3

...  Binary stars are when there are two stars and they revolve around each other.  In these systems supernovas occur also.  Stars up to eight times the mass of our sun usually evolve into white dwarfs.  A star that is condensed to this size has a very strong gravitational pull.  With that gravity, ...
FREE Sample Here
FREE Sample Here

... appears to us when viewing the star from here on Earth. Apparent visual magnitude does not take into account any corrections for the star's distance, size, temperature, or the amount of dust between us and the star. It is simply the brightness as it appears to us in the night sky. ...
C H A P T E R  2
C H A P T E R 2

... appears to us when viewing the star from here on Earth. Apparent visual magnitude does not take into account any corrections for the star's distance, size, temperature, or the amount of dust between us and the star. It is simply the brightness as it appears to us in the night sky. ...
Studying the Stars
Studying the Stars

... Pogson assigned the brightest stars the first order of magnitude (magnitude = 1), and dimmer stars were 2nd, 3rd, 4th order, etc. (magnitudes = 2, 3, 4, etc.) Now that we can be more accurate in our measurements, stars can have more specific magnitudes like 1.5, 6.73, etc. and even negative numbers ...
Atoms and Stars IST 3360 and IST 1990
Atoms and Stars IST 3360 and IST 1990

... • on a sphere, angles of a triangle add up to less than 360º ...
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