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08Moon - NMSU Astronomy
08Moon - NMSU Astronomy

IV International Astronomy Olympiad
IV International Astronomy Olympiad

... diameter in the objective focal plane if its focal length is 254 cm and the objective diameter is 40 cm? Draw a figure (a few figures) to explain your calculations. 2. A photometer is mounted on a 125 cm (focal length) telescope. Can you observe a star with magnitude a. 5m b. 10m c. 15m in a cluster ...
Quick Reference - Objects in the skies
Quick Reference - Objects in the skies

... These are patterns formed by prominent stars within apparent proximity to one another on Earth's night sky. There are 88 standard constellations recognized by the International Astronomical Union (IAU) since 1922. The majority of these go back to the 48 constellations defined by Ptolemy in his Almag ...
planets orbit around Sun.
planets orbit around Sun.

... Kepler, using Brahe's detailed observations, realized that the planets moved around the sun not in circles but in stretched out circles known as ellipses. However, the problem took him almost a decade to solve, and Kepler didn't publish it until well after Brahe's death. Although Brahe's family inte ...
Scaling the SEM reading
Scaling the SEM reading

... approximately 4.5 billion years ago. The debris from that collision was thrown out into space, and that debris eventually joined together to form the Moon. The newly formed Moon traveled at just the right speed so that it remained within the control of Earth’s gravitational field. Now the Moon is Ea ...
Advanced Solar Theory (MT5810)
Advanced Solar Theory (MT5810)

Quiz Questions
Quiz Questions

... 3. We feel sure that the sun is now fueled by nuclear energy rather than by energy left over from its gravitational contraction because A. we don't see the sun contracting B. the spectrum looks like nuclear production C. the energy from gravitational contraction can't last long enough D. we see heli ...
Age and Origin of the Earth
Age and Origin of the Earth

Planetary Cycles Witness To The Creator
Planetary Cycles Witness To The Creator

Slide 1
Slide 1

... •The sun, Earth and its moon are spherical objects that move in two ways: They spin (rotate) and they change positions relative to each other (revolve). •Places on the earth experience seasons, providing evidence that the earth is revolving around the sun. •The sun is a star that produces light that ...
Planet Powerpoint
Planet Powerpoint

... huge storm of swirling gas that has lasted for hundreds of years. Jupiter does not have a solid surface. The planet is a ball of liquid surrounded by gas. ...
The Motions of Celestial Bodies, and Newton`s Laws of Motion
The Motions of Celestial Bodies, and Newton`s Laws of Motion

... 2. As a planet moves around it’s orbit, it sweeps out equal areas in equal times. ...
Minor Members of the Solar System
Minor Members of the Solar System

... 23.4 Minor Members of the Solar System Asteroids: Microplanets  An asteroid is a small, rocky body whose diameter can range from a few hundred kilometers to less than a kilometer.  Most asteroids lie between the orbits of Mars and Jupiter. They have orbital periods of three to six years. ...
Study guide
Study guide

The New Cosmology: Our Expanding Universe
The New Cosmology: Our Expanding Universe

... and ideological reasons, the problem was that every movement could be explained by means of epi-circles, depending on how big one made the circle and how many of them one invented to do the job. Copernicus realized that placing the sun in the center of the universe, and the planets orbiting this cen ...
The New Cosmology: Our Expanding Universe
The New Cosmology: Our Expanding Universe

... and ideological reasons, the problem was that every movement could be explained by means of epi-circles, depending on how big one made the circle and how many of them one invented to do the job. Copernicus realized that placing the sun in the center of the universe, and the planets orbiting this cen ...
A new Cosmos – a novel Physics
A new Cosmos – a novel Physics

Star clusters and constellations
Star clusters and constellations

... Star clusters are groups of stars that are ‘connected’ by a significant gravitational force ands move around tougher as the galaxy rotates. The motion of the Sun through the galaxy does not affect the appearance of a star cluster from Earth over a long period of time. Examples of star clusters are t ...
PowerPoint Presentation - Planetary Configurations
PowerPoint Presentation - Planetary Configurations

... Interaction of Matter and Light • Absorption: Occurs when a photon of the correct energy moves an electron from a lower orbit to an upper orbit. • Emission: Occurs when an electron drops from an upper orbit to a lower one, thereby ejecting a photon of corresponding energy • Ionization: Occurs when ...
Article - Iowa State University
Article - Iowa State University

... moon Charon remains a moon. The IAU lists at least a dozen more solar bodies that could fall into the dwarf planet category in the coming months and years. Kerton says that although Pluto’s status seems like a demotion, it shouldn’t. “The language of Pluto being demoted and losing its status is only ...
Name
Name

Application Exercise: Distances to Stars Using Measured Parallax
Application Exercise: Distances to Stars Using Measured Parallax

... four basic methods of determining distances: radar, parallax, standard candles, and the Hubble Law. Each of these methods is most useful at certain distances, with radar being useful nearby (e.g., the Moon), the Hubble Law being useful at the farthest distance (e.g., galaxies far, far away). In this ...
The Parsec
The Parsec

... small angle, just below Star A, formed by the two longest sides of this triangle is called the parallax angle for Star A. Label this angle “pA.” Knowing a star’s parallax angle allows us to calculate the distance to the star. Since even the nearest stars are still very far away, parallax angles are ...
The Sun`s Exterior
The Sun`s Exterior

... Above the chromosphere is the corona, the faint halo visible around the Sun during an eclipse. The corona is extremely hot: 1 million Kelvin. But it is also very low density. It does not produce much light of its own, but scatters sunlight very strongly. (Image credit: Fred Espenak) ...
properties of stars 2012
properties of stars 2012

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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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