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Understanding Precession of the Equinox
Understanding Precession of the Equinox

... Gregorian Calendar change (420 years ago), thereby causing the equinox to drift about 5.9 days. This has not happened; the equinox is stable in time after making leap adjustments. Therefore, it was theorized that the equinox must slip about 50 arc seconds per year along the ecliptic and the equinoct ...
Astronomy 730 / Galaxies
Astronomy 730 / Galaxies

... zb. At t = t0 the boundary conditions are that σz(R, t0) = σz(0, t0) exp(−R/2hR) and hz(R, t0) = constant. If we take σz(R0,t0) = 20 km/s, we know that hz(R, t0) = 350 pc, again based on the old stars in the thin disk in the solar neighborhood. (c) Equate σz(R, t0) = σz(0, t0) exp(-R/2hR) with σz(R, ...
Celestial Sphere
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... 1) Is the horizon shown a real physical horizon, or an imaginary plane that extends from the observer and Earth out to the stars? ...
ChAPTER 10 sTARS
ChAPTER 10 sTARS

... 2. Proxima Centauri, is closer to Earth it would appear to shift the greatest distance when compared to the background stars. Similarly, Alpha Centauri, would shift less. This is because as a star’s distance from Earth increases, its parallax angle decreases, causing the shift in position to appear ...
KS1 Education Guide - Immersive Theatres
KS1 Education Guide - Immersive Theatres

... solar system Star – a: a natural luminous body visible in the sky especially at night b: a self-luminous gaseous spheroidal celestial body of great mass which produces energy by means of nuclear fusion reactions Sun – the luminous celestial body around which the earth and other planets revolve, from ...
Coordinate Systems - AST 114, Astronomy Lab II for Spring 2017!
Coordinate Systems - AST 114, Astronomy Lab II for Spring 2017!

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fifth midterm -- review problems

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Abundances of RGB stars in NGC 6752 Grundahl

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Review: How does a star`s mass determine its life story?

... (about 10 thousand times)!!! • Nova: H to He fusion of a layer of accreted matter, white dwarf left intact • Supernova: complete explosion of white dwarf, nothing left behind © 2010 Pearson Education, Inc. ...
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Massive stars as thermonuclear reactors and their explosions

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... 2. Microlensing on isolated stellar mass BHs • There are several good candidates • But it is necessary to find the black hole ITSELF! 3. Exotic emission mechanisms • As all other exotics: interesting, but not very probable • If it works, then GLAST will show us isolated BHs 4. Runaway stars • A rare ...
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... 2. Microlensing on isolated stellar mass BHs • There are several good candidates • But it is necessary to find the black hole ITSELF! 3. Exotic emission mechanisms • As all other exotics: interesting, but not very probable • If it works, then GLAST will show us isolated BHs 4. Runaway stars • A rare ...
Explosion of Sun - Scientific Research Publishing
Explosion of Sun - Scientific Research Publishing

mufon ufo symposium -1974
mufon ufo symposium -1974

... sequence stars in the best range for life in a 10 parsec radius of Earth were probably variable, although I could find no reason why the percentage is so high. The ratio dropped to 1/20 in the 10 to 20 parsec range, so we probably are not catching the variability in these stars. If the star is varia ...
Table of Contents - Imiloa Astronomy Center
Table of Contents - Imiloa Astronomy Center

... - This huge star has a radius that is probably almost 4 AU. - If the sun were replaced by Antares A at the center of the solar system, the earth would be engulfed, as would be Mars and the Asteroid Belt. - It is also estimated to be about 600 years away. - Antares companion is usually described as g ...
Are Gamma-Ray Bursts good Star Formation Indicators?
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... environmental dependence of GRB rate or luminosity which is hard to account for. Indeed there is some evidence of such a metallicity dependence (see below). Some GRBs may be so heavily enshrouded in dust that we only detect their gamma-rays, making redshift estimates more uncertain. GRBs are short l ...
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classifying stars

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... Through a process called accretion (i.e., sticky collision) dust particles in the disk steadily accumulate mass to form ever-larger bodies. Local concentrations of mass known as planetesimals begin to form, and these accelerate the accretion process by drawing in additional material by their gravita ...
astronomy - Jiri Brezina Teaching
astronomy - Jiri Brezina Teaching

... relationship between heat and other forms of energy), ELECTROSTATICS & ELECTRODYNAMICS, MAGNETOSTATICS and MAGNETODYNAMICS. Modern physics is concerned with the behavior of matter and energy under extreme conditions or on the very large or very small scale. For example, atomic and nuclear physics st ...
Chapter 4 The Origin and Nature of Light
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... ifferent people perceive the Sun to have different colors. To many it appears white, to others yellow. Still others, who notice it at sunset, believe it to be orange or even red. But we have seen that the Sun actually gives off all colors. Moreover, the peak in the Sun’s spectrum falls between blue ...
"The Sun Is A Plasma Diffuser That Sorts Atoms By Mass"
"The Sun Is A Plasma Diffuser That Sorts Atoms By Mass"

... the likely carrier of s-products just found in Os from unequilibrated chondrites [42]. c.) (SiO2, #Z =11): Silicates are abundant and show few anomalies in meteorites. A component of “almost pure ...
The surface composition of Beta Pictoris
The surface composition of Beta Pictoris

... isolated line, and serving as a measure of line strength. They are denoted less certain if the ‘target’ line is not the dominant contributor to a spectral feature (but is still clearly traceable). The stellar microturbulent velocity ξ was determined as usual by comparing abundances derived from vari ...
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IK Pegasi



IK Pegasi (or HR 8210) is a binary star system in the constellation Pegasus. It is just luminous enough to be seen with the unaided eye, at a distance of about 150 light years from the Solar System.The primary (IK Pegasi A) is an A-type main-sequence star that displays minor pulsations in luminosity. It is categorized as a Delta Scuti variable star and it has a periodic cycle of luminosity variation that repeats itself about 22.9 times per day. Its companion (IK Pegasi B) is a massive white dwarf—a star that has evolved past the main sequence and is no longer generating energy through nuclear fusion. They orbit each other every 21.7 days with an average separation of about 31 million kilometres, or 19 million miles, or 0.21 astronomical units (AU). This is smaller than the orbit of Mercury around the Sun.IK Pegasi B is the nearest known supernova progenitor candidate. When the primary begins to evolve into a red giant, it is expected to grow to a radius where the white dwarf can accrete matter from the expanded gaseous envelope. When the white dwarf approaches the Chandrasekhar limit of 1.44 solar masses (M☉), it may explode as a Type Ia supernova.
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