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1 The Solar System - e
1 The Solar System - e

... Have you carefully observed the sun, moon and the other celestial bodies in the sky? There is evidence that man had shown an interest in knowing about them since ancient times. At present man can explore more than what is visible to the naked eye, as scientists have invented modern equipment to obs ...
HOMEWORK #1
HOMEWORK #1

... Just as brightness is related to apparent magnitude, luminosity is related to a term called “absolute magnitude.” Astronomers refer to a star’s “absolute magnitude (M)” as the apparent magnitude it would have at an arbitrary standardized distance of 10 parsecs (i.e., 32.6 light-years). #2. Combine ...
White Dwarf Stars Near The Earth
White Dwarf Stars Near The Earth

... the chart, Sirius B is unusually hot, and that means it is unusually young, probably only 250 million years or thereabouts. It is also unusually massive, being the remnant of a giant B-class star that probably weighed in at over five solar masses when it was born. Procyon B is the companion to Procy ...
Word
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... Just as brightness is related to apparent magnitude, luminosity is related to a term called “absolute magnitude.” Astronomers refer to a star’s “absolute magnitude (M)” as the apparent magnitude it would have at an arbitrary standardized distance of 10 parsecs (i.e., 32.6 light-years). #2. Combine ...
The Night Sky This Month - Usk Astronomical Society
The Night Sky This Month - Usk Astronomical Society

... in the constellation, the red giant star Aldebaran, is prominent in the vee and is described as the right eye of the bull, even though its name means the ‘follower’ of the Pleiades in medieval Arabic. As an open cluster many of these stars have similar distances and are moving with similar proper mo ...
Robotics - UNL CSE
Robotics - UNL CSE

... men on other planets. If you can imagine that, then you are seeing Kepler, NASA’s alienfinding telescope, burst into space on March 6. The Kepler Project has many parts, including processing the never-ending stream of data and finding the planets in the first place. On March 6, 2009, Kepler was laun ...
BENNETT, Constraints on the Orbital Motion of OGLE-2006
BENNETT, Constraints on the Orbital Motion of OGLE-2006

... – Slight dependence on distance to the source star when converting to physical from Einstein Radii units ...
PLANETARY MOTIONS
PLANETARY MOTIONS

... planets for several years, we will use a mechanical device, the orrery to represent planetary motions in an accelerated fashion. An orrery is a mechanical model of the Solar System. The model Sun is at the center and the model planets are driven around by a system of gears. Sometimes, on more elabor ...
Earth in Space
Earth in Space

... Some astronomers think the Moon may have been formed when a Mars-sized asteroid collided with Earth about 100 million to 200 million years after Earth was formed approximately 4.5 billion years ago. The debris from that collision was thrown out into space, and that debris eventually joined together ...
Powerpoint for today
Powerpoint for today

... (amount of energy put out every second in form of radiation). Luminosity also called “absolute brightness”. How bright a star appears to us is the “apparent brightness”, which depends on its luminosity and distance from us: apparent brightness ...
Astronomy, Chapter 1 Learning Target #1 Explain the motion of the
Astronomy, Chapter 1 Learning Target #1 Explain the motion of the

... a) Identify the moon’s cycle in relationship to a month on Earth (full moon, new moon) using diagrams b) Explain how many days it takes for a moon to go through one cycle …such as how long it would take for a new moon or full moon to occur during the next cycle c) Compare/contrast a solar and lunar ...
Solar System - HMXEarthScience
Solar System - HMXEarthScience

... C) They exert the same gravitational force on each other. D) They have elliptical orbits with the Sun at one focus. 37. The actual shape of the Earth's orbit around the Sun is best described as A) a very eccentric ellipse C) an oblate spheroid ...
Abs-Apar Mag
Abs-Apar Mag

... • 1856 proposal to standardize • standard ratio of 2.512 between magnitudes. • 5 magnitude steps correspond to 100x factor brightness change • The Star Vega selected as baseline (magnitude 0.0) – 5th brightest star, 2nd in North hemisphere – Is now magnitude 0.03, by redefined baseline scale ...
Earth, Sun and Moon model
Earth, Sun and Moon model

... The Sun is a star found at the centre of our Solar System. It makes up around 99.86% of the Solar System’s mass. The light from the Sun takes around 8 minutes to reach the Earth. Other stars may be larger, brighter, smaller or fainter than our Sun but they are so very far away that we only see them ...
Astronomy 103: Midterm 2 Answers Correct answer in bold
Astronomy 103: Midterm 2 Answers Correct answer in bold

... 34. Two clouds of interstellar gas contract to form stars. Suppose that no mass is lost in the contraction and that when they stop contracting, cloud A is a type A star and cloud K is a type K star. What stops the contraction of each star? ...
Cosmic distance scales - Inside Mines
Cosmic distance scales - Inside Mines

... Physics Department, Colorado School of Mines ...
Mission 1: What`s In Our Sky
Mission 1: What`s In Our Sky

Astronomy Library wk 6.cwk (WP)
Astronomy Library wk 6.cwk (WP)

... e.g. how would you measure the length of a table? Is this enough? We have seen how stellar spectra can be used to determine stellar composition and temperature. Here we will see how we can determine some other stellar properties: Luminosity: Energy emitted by a star per unit time. Radius of a star ...
The formation of stars and planets
The formation of stars and planets

Chapter 08
Chapter 08

... Protons need large velocity (high temperature) to overcome Coulomb barrier (electrostatic repulsion between protons). ...
Carbon Dioxide and Long
Carbon Dioxide and Long

... • Hypothesis that life evolved in order to regulate Earth’s climate • Named after the Greek Goddess known as Earth or Mother Earth (the Greek common noun for "land" is ge or ga). • It is written that Gaia was born from Chaos, the great void of emptiness within the universe ...
4-3 Astronomy
4-3 Astronomy

... atmosphere, and location; therefore, the primary focus of assessment should be to detect ways that these objects are alike and different. However, appropriate assessments should also require students to identify the object based on its description; or illustrate the objects by their location in the ...
2008oct23
2008oct23

The Planets
The Planets

... The Planets and the Solar System The Solar System Planet – is a celestial body that orbits one or more stars. Planets only reflect light radiated by its star, they do NOT generate their own energy. Solar System – a group of planets circling one or more stars Each galaxy spins around a central nucle ...
Measuring the Stars
Measuring the Stars

... actual shift of the star in the sky, after correcting for parallax These pictures were taken 22 years apart: ...
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Astronomical unit

The astronomical unit (symbol au, AU or ua) is a unit of length, roughly the distance from the Earth to the Sun. However, that distance varies as the Earth orbits the Sun, from a maximum (aphelion) to a minimum (perihelion) and back again once a year. Originally conceived as the average of Earth's aphelion and perihelion, it is now defined as exactly 7011149597870700000♠149597870700 meters (about 150 million kilometers, or 93 million miles). The astronomical unit is used primarily as a convenient yardstick for measuring distances within the Solar System or around other stars. However, it is also a fundamental component in the definition of another unit of astronomical length, the parsec.
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