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Nearest star`s wobbles could reveal Earth`s twin
Nearest star`s wobbles could reveal Earth`s twin

... should be able to pick up the slight stellar wobbles induced by a small, rocky, Earth-like planet. Alpha Centauri lies just over 4 light years away and is the closest star system to the Sun. It appears to be a triple system, with two Sun-like stars orbiting each other relatively closely (about 23 ti ...
Deep-sky-object hunter
Deep-sky-object hunter

... models each run about $100 less. The truss variation of the Dobsonian mount makes large telescopes more portable by breaking down their elements into compact packages. But until Meade started mass-producing them, only high-end or homemade Dobs used the truss design. In other words, to find a truss t ...
Integrative Studies 410 Our Place in the Universe
Integrative Studies 410 Our Place in the Universe

... • Sun’s life expectancy ~ 10 billion (1010) years • Careful study of the Sun ~ 370 years • We have studied the Sun for only 1/27 millionth of its lifetime! ...
August 2013 - Joliet Junior College
August 2013 - Joliet Junior College

In the Spring of 2007 two of us began planning a new course in
In the Spring of 2007 two of us began planning a new course in

... d. mass e. chemical makeup 15. Current evidence about how the universe is changing tells us that a. We are near the center of the universe. b. Galaxies are expanding into empty space. c. Groups of galaxies appear to move away from each other d. Nearby galaxies are younger than distant galaxies. 16. ...
Lecture 12
Lecture 12

... Can determine the distance directly if we can measure the ...
How to Buy an Astronomical Telescope
How to Buy an Astronomical Telescope

... movement straight up and down and side to side – usually by hand power. Aperture: the effective diameter (expressed in either ...
Physics of Astronomy – Week 3 quiz
Physics of Astronomy – Week 3 quiz

... A person with good vision can resolve details as small as 1 arminute. Could this person resolve the crescent of Venus with naked eye? Explain. Since the size of Venus is smaller than the smallest angle a good eye can resolve, the crescent of Venus cannot be resolved by naked eye (despite anecdotes t ...
PARTS LIST FOR AT50 Telescope
PARTS LIST FOR AT50 Telescope

... Each of the planets provides interesting views. Venus is covered with clouds so all that is visible is an extremely bright light, the brightest next to the moon. However, Venus, like the moon, goes through phases. As it travels around the sun, different areas of its surface are illuminated, producin ...
The Prehistory and Cryptozoology of the Telescope
The Prehistory and Cryptozoology of the Telescope

... closer than its center of curvature. ● To put the center of curvature at the distance of a ship would require a mirror many meters tall. ● In this period mirror makers were producing accurate curves on the order of centimeters, not meters. ...
Telescopes - Wayne State University Physics and Astronomy
Telescopes - Wayne State University Physics and Astronomy

... the National Radio Astronomical Observatory's Very Large Array (VLA) near Socorro, New Mexico It consists of 27 movable radio telescopes, each having an aperture of 25 m, spread over a total span of about 36 km The telescopes signals are combined electronically and permit astronomers to obtain pictu ...
File - Mr. Gray`s Class
File - Mr. Gray`s Class

... – Planets normally move westward across the night sky. This is called Prograde motion. – Sometimes planets appear to begin moving “backward” or eastward across the night sky. This is called Retrograde motion.  Please not that if you look these words up, the directions will be backwards because Astr ...
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NASA Discovers The Entire New Solar System Called

... planetary system, located 12 parsecs away from the Solar system (39 light years), near the ecliptic, within the constellation of Aquarius. Around a star which is 12 times less massive than the Sun and only slightly larger than Jupiter, there are at least seven planets in orbit. The initial discovery ...
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... Telescopium constellation lies in the southern sky, to the south of Sagittarius and Corona Australis. It represents a telescope The constellation culminates on the 13th of August, at the same time as Wega (Vega) of the Lyre (Lyra). Telescopium is the 57th constellation in size, occupying an area of ...
Basics of Astrophysics
Basics of Astrophysics

Thursday October 1 - Montana State University
Thursday October 1 - Montana State University

... • Luminosity means total power output as light. • Determining their distance from us would be easy if they all were the same luminosity! ...
What`s Up - April 2016
What`s Up - April 2016

... At about 40 times the diameter of the sun and 400 times as bright, Alphard is one of the ‘bright giants’ in our neighbourhood. But our ‘neighbourhood’ is rather large. Alphard is 11 million times as far away from us as our own sun – so it looks a lot dimmer to us! To the south of Sirius, and nearly ...
Chapter 13: Interstellar Matter and Star Formation
Chapter 13: Interstellar Matter and Star Formation

... (i) Absorption lines due to interstellar gas tend to be narrower than those produced by a star’s atmosphere. (ii) Lines caused by a stellar atmosphere will have a different Doppler shift than those caused by the interstellar gas. (iii) Interstellar gas will generally be much cooler than the gas of t ...
The Death of Stars
The Death of Stars

... • Perhaps the most famous is the “Crab Nebula” from a supernova in 1054 AD. It was so bright, Chinese, Japanese, and Arab astronomers saw it for months during the day, and could be seen for 2 years at night. • The remnant merges with other gas and forms new stars. • Supernovae occur 1 to 3 times per ...
Fulltext PDF - Indian Academy of Sciences
Fulltext PDF - Indian Academy of Sciences

... Of whose true fixed and resting quality There is no fellow in the firmament. One important practice of scientists is to keep a log of what they do and observe. Nowhere has this been done with greater devotion than in astronomy where, since ancient times, one has been keeping accurate records of the ...
look-back time exercise[1][2]
look-back time exercise[1][2]

... The goal of this laboratory exercise is to introduce the student to the concept of look-back time. Because the speed of light is not infinitely fast, the light from distant objects takes time to reach us here on Earth. At the end of this lab, the students should have greater appreciation of how this ...
Jupiter, the fifth planet from the sun and the largest planet in our
Jupiter, the fifth planet from the sun and the largest planet in our

... The other source of comets is a debris cloud of ice, possibly left over from the formation of the solar system, called the Oort Cloud. Scientists study comets because it helps them learn about the origin of the Solar System. Historically, comets have been considered omens of bad times such as the de ...
What We Know About Stars So Far
What We Know About Stars So Far

... color of the star told us something about their temperature •Red-colored stars are cooler in temperature compared to bluecolored stars. ...
The universe is faster, colder, and wackier than anything we can
The universe is faster, colder, and wackier than anything we can

... of space such that they can move without being affected by larger galaxies, they can reach out with their feeble gravity and take up a fragile orbit around each other. Of the many binary pairs of small galaxies we know of, the pair that is bound together most weakly is an obscure duo known as SDSS J1 ...
Pythagoras Eudoxus of Cnidus Aristotle Eratosthenes Hipparchus
Pythagoras Eudoxus of Cnidus Aristotle Eratosthenes Hipparchus

... Brahe Tycho Brahe was born December 14, 1546 in Denmark. He studied law but became interested in astronomy when he observed a solar eclipse in 1560. He read Ptolemy’s Almagest and went on to study science in several universities. In 1572, Brahe discovered a nova (a star that becomes very bright then ...
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International Ultraviolet Explorer



The International Ultraviolet Explorer (IUE) was an astronomical observatory satellite primarily designed to take ultraviolet spectra. The satellite was a collaborative project between NASA, the UK Science Research Council and the European Space Agency (ESA). The mission was first proposed in early 1964, by a group of scientists in the United Kingdom, and was launched on January 26, 1978 aboard a NASA Delta rocket. The mission lifetime was initially set for 3 years, but in the end it lasted almost 18 years, with the satellite being shut down in 1996. The switch-off occurred for financial reasons, while the telescope was still functioning at near original efficiency.It was the first space observatory to be operated in real time by astronomers who visited the groundstations in the United States and Europe. Astronomers made over 104,000 observations using the IUE, of objects ranging from solar system bodies to distant quasars. Among the significant scientific results from IUE data were the first large scale studies of stellar winds, accurate measurements of the way interstellar dust absorbs light, and measurements of the supernova SN1987A which showed that it defied stellar evolution theories as they then stood. When the mission ended, it was considered the most successful astronomical satellite ever.
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