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UNIT TWO Astronomical Instruments and Light
UNIT TWO Astronomical Instruments and Light

... 47. The _____________ of a star can be determined from its color. 48. The process of removing an electron from a stable nucleus is known as ____________. 49. ___________ is a measure of the amount of energy due to the motion of the particles in a gas. liquid, or solid. 50. If one star has a temperat ...
ppt
ppt

... • Mercury: never farther than 27 degrees from the sun, on morning or evening side • Venus: never farther than 47 degrees from the sun, on morning or evening side • Mars, Jupiter, Saturn: move eastward within the zodiac, but each one makes a westward loop once a year when its farthest from the sun •U ...
Our Universe
Our Universe

... moving away from Earth, its electromagnetic spectrum stretches; the result is that wavelengths appear longer and shift toward the red end of the spectrum. ...
IMAGES FROM SPACE
IMAGES FROM SPACE

Motions of the Planets: Not the same as Stars!
Motions of the Planets: Not the same as Stars!

... •  Mercury: never farther than 27 degrees from the sun, on morning or evening side •  Venus: never farther than 47 degrees from the sun, on morning or evening side •  Mars, Jupiter, Saturn: move eastward within the zodiac, but each one makes a westward loop once a year when its farthest from the sun ...
The Stars
The Stars

... The Stars Stars vary greatly in size, brightness, temperature, and colour. Here are some of the things we have learned about the properties of stars. Measuring distance Just as with the kilometre, the AU is not very useful when we start to study stuff outside of our Solar System. A much larger unit ...
11.1 Stars - St John Brebeuf
11.1 Stars - St John Brebeuf

... See pages 368 - 369 ...
Extension worksheet – Topic 6 - Cambridge Resources for the IB
Extension worksheet – Topic 6 - Cambridge Resources for the IB

... Draw lines on the diagram to show the evolutionary paths of stars X and Y. ...
- Microsoft Research
- Microsoft Research

... Summarizing, Analyzing, Visualizing ...
The Fates of Stars Mass-Luminosity Relation: Lifetime Relation:
The Fates of Stars Mass-Luminosity Relation: Lifetime Relation:

... spectral class ...
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Earth`s Atmosphere & Telescopes
Earth`s Atmosphere & Telescopes

... everyone’s ability to enjoy the night sky. • The atmosphere scatters light from cities over long distances • Astronomers must go to remote locations to make observations ...
Optical Telescope
Optical Telescope

... Telescope CCDs • CCDs are sensitive to light from ultraviolet to infrared. ...
What is a Solar System?
What is a Solar System?

... as Dawn mission approaches Ceres this month ...
Stars from Afar
Stars from Afar

... Stars can be classified in three ways: Size – How massive the star is  Temperature – A stars color reveals its temperature. ...
Stars and The Universe
Stars and The Universe

... Stellar Evolution: The Deaths of Stars a. A Second Red-Giant Phase ...
History of the Universe and Solar System
History of the Universe and Solar System

... No, gravitational forces have slowed down the galaxies since the Big Bang. (Note: Recent observations suggest this was the case for the first 2/3 of the Universe’s history. The expansion rate now seems to have increased for the last 1/3 of the Universe’s history. This is explained by “dark phantom e ...
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File

... A unit used to measure long distances, equivalent to the distance from the Sun to Earth, is known as the: a. light year. b. cosmic scale. c. astronomical unit. d. sidereal year. ...
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... percent in a specific time period, and “n” is the total number of those periods that have elapsed. For example, "Moore's law" is the empirical observation that, over the history of modern computer technology, the number of transistors in an integrated circuit doubles approximately every two years. U ...
HOMEWORK #1
HOMEWORK #1

... percent in a specific time period, and “n” is the total number of those periods that have elapsed. For example, "Moore's law" is the empirical observation that, over the history of modern computer technology, the number of transistors in an integrated circuit doubles approximately every two years. U ...
Document
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... Looking up at the night sky, you won’t see the sun and all the planets that belong to our solar system, but you may see the moon and some stars. Long ago, people thought the stars made patterns in the sky that looked like people, animals, and other things. These groups of stars were called constell ...
LOFT_group_developme.. - LOFT, Large Optics Fabrication and
LOFT_group_developme.. - LOFT, Large Optics Fabrication and

... 3.2-m segmented secondary mirror corrects for PM position errors deformable mirror for adaptive optics ...
ScienceHelpNotes-UnitE1 - JA Williams High School
ScienceHelpNotes-UnitE1 - JA Williams High School

... describing the position of objects in space, using angular coordinates (e.g., describe the location of a  spot on a wall, by identifying its angle of elevation and its bearing or azimuth; describe the location of  the Sun and other stars using altitude­azimuth coordinates, also referred to as horizo ...
stars and galaxies – study guide
stars and galaxies – study guide

... 2. Most stars are composed mainly of what two elements? hydrogen and helium. 3. If a star’s spectral lines are shifted towards the red end of the spectrum, then the star is moving away from the Earth. 4. Objects moving closer to the Earth, shift the spectrum to the blue end. 5. The part of the elect ...
The night sky - Mr. Champion
The night sky - Mr. Champion

... a clear night and noticed patterns and changes. • Humans have for many years speculated at what was above us. • This is the study of astronomy – what is beyond Earth. • The first would likely be the most numerous object we see – stars. ...
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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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