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The Bigger Picture
The Bigger Picture

Tuesday, October 28th "The Formation and Evolution of Galaxies"
Tuesday, October 28th "The Formation and Evolution of Galaxies"

... "That may sound like a very small angle, but it is in fact significant," says Alexei Pevtsov, RHESSI Program Scientist at NASA Headquarters. Tiny departures from perfect roundness can, for example, affect the Sun's gravitational pull on Mercury and skew tests of Einstein's theory of relativity that ...
Excerpts - Solar and Sidereal Time
Excerpts - Solar and Sidereal Time

... one hundred minutes, and the minute into a hundred seconds, because of the facility in computation, and in conformity with their decimal system of weights and measures. This subdivision is not now used in common life, nor has it been adopted in any other country; and although some scientific writers ...
Seasonal Visibility of Stars, and Visibility of Planets in 2014
Seasonal Visibility of Stars, and Visibility of Planets in 2014

PDF
PDF

... 2. An imaginary line drawn throught the earth from the North to the South pole. 3. This planet is between Saturn and Neptune. 4. A sun seen from a great distance. 6. On earth the sun appears to rise in the ___. 7. Gravity on this is one sixth of what it is on earth. It takes 28 days to go round the ...
DOCX
DOCX

... moon are the same size, each about 32 miles in diameter, and less than 3,000 miles above the earth. The sun is not a star and the 'planets' are not physical (rocky or gaseous) bodies but wandering stars. We have night and day because sunlight is localized and does not travel indefinitely. It has a r ...
X-RAY OBSERVATIONS OF SEYFERT GALAXIES The dawn of a …
X-RAY OBSERVATIONS OF SEYFERT GALAXIES The dawn of a …

... position did not change (so it was not a comet or meteor), - lack of Parallax must be in one of the “outer spheres” -therefore the outer sphere of stars does change! a Comet position did not change significantly throughout the night. - lack of Parallax, must lay beyond the orbit of the Venus Observe ...
General Astronomy - Stockton University
General Astronomy - Stockton University

... Polaris. As the evening passes, the stars appear to rotate clockwise about Polaris. • For a given latitude of an observer, some stars never set - these are known as circumpolar stars • If you were at the North Pole, Polaris would be nearly on your zenith and the motion of the stars would be parallel ...
Answer - Physics@Brock
Answer - Physics@Brock

... 49. The cycle of the Moon’s phases repeats approximately once every (a) day. (b) 29.5 days. (c) six months. (d) year. 50. The constellations of the Zodiac lie along the (a) ecliptic. (b) celestial equator. (c) celestial seasonings. (d) celestial tuning fork. ...
Answers - Physics@Brock
Answers - Physics@Brock

... 49. The cycle of the Moon’s phases repeats approximately once every (a) day. (b) * 29.5 days. (c) six months. (d) year. 50. The constellations of the Zodiac lie along the (a) * ecliptic. (b) celestial equator. (c) celestial seasonings. (d) celestial tuning fork. ...
Components of the Solar System Learning Targets
Components of the Solar System Learning Targets

... Target 4: Gravity holds the planets in orbit around the sun and the fact that the planets want to travel in a straight line (inertia) Because the sun makes up 99% of the solar system’s mass, it has a very large gravitational pull that holds the planets and other objects in orbit. Target 5: The Galil ...
Second Lecture - University of Maryland Astronomy
Second Lecture - University of Maryland Astronomy

... • Lived and observed on island off the coast of Denmark • Last of the great “naked eye” observers • Made planetary observations much more accurate than any previous… first to estimate error bar of a measurement • Observed “new star” (Tycho’s supernova; 1572) • Demonstrated that comet was beyond Moon ...
Subject: Earth Science Grade: 11 Unit #: 1 Title: Astronomy
Subject: Earth Science Grade: 11 Unit #: 1 Title: Astronomy

... Students will participate in a debate, or generate an argument that is recorded as a podcast, script or radio broadcast regarding possible influences objects from space can have on Earth. The debate or podcast will include information about how Earth’s solar system formed and changed over time, Eart ...
Chapter 8 Powerpoint
Chapter 8 Powerpoint

... some bacteria were found fossilized in a fragment of rock from Mars. ...
4 The Sun
4 The Sun

... Now that we have all the theoretic building blocks in place, let’s start using them by having a look at our central star, the Sun: Mass Radius Distance Age Escape velocity ...
Homework 12 1. How would phases change if the Moon were the
Homework 12 1. How would phases change if the Moon were the

... 3. How would eclipses change if the Moon were the same size as Earth, but still had the same mass? Both total and partial solar eclipses would be more frequent because there is a greater chance that the larger Moon would block the Sun. The Earth will have more Moon to block, but a bigger target. The ...
Planets around Other Stars
Planets around Other Stars

... Reproduced below is a plot of observations of the radial velocity of the star 51 Pegasi, the first star discovered to have a planet. The observed velocity (in meters per second) is plotted vs. the time (in days) when the observation was made. The velocity of the star varies with time because the sta ...
Seasons and the Changing Sky
Seasons and the Changing Sky

... •  On the sky: ...
the planets - St John Brebeuf
the planets - St John Brebeuf

... 2) Luckily, our magnetic field deflects this solar wind. We can see these particles being deflected when we see the Northern Lights. 3) Large outbursts of solar winds can wreak havoc with satellites as well as Earth-bound energy supplies such as power plants. ...
the planets - St John Brebeuf
the planets - St John Brebeuf

... 2) Luckily, our magnetic field deflects this solar wind. We can see these particles being deflected when we see the Northern Lights. 3) Large outbursts of solar winds can wreak havoc with satellites as well as Earth-bound energy supplies such as power plants. ...
MULTIPLE CHOICE QUESTIONS (50 pts
MULTIPLE CHOICE QUESTIONS (50 pts

... B. using its distance from the Sun and its rotational period. C. using its angular size and distance from Earth. D. using data from spacecraft flybys. E. by measuring the time that it takes for the Red Spot to disappear from view. 21. Today the Sun physically dips below the horizon at 7:52 PM EDT. H ...
Apparent Motions of Celestial Objects
Apparent Motions of Celestial Objects

File - Mr. Dudek`s Science
File - Mr. Dudek`s Science

... found that they were ellipses. • He also learned that the speed of each of the planets was different and the outer planets took much longer to orbit the Sun (Mercury=88 days, Saturn= 29.5 years). ...
Describe essential ideas about the composition and structure of the
Describe essential ideas about the composition and structure of the

The energy budget of planets
The energy budget of planets

... Additional complication: Solar luminosity changes with time (slowly)… Sun was less luminous in the past and is slowly getting more luminous Faint Sun problem: initial Solar luminosity is predicted to be ~70% of the current luminosity… but no evidence that temperature on the early Earth was much col ...
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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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