OLEARY_2004 - Armagh Observatory
... In order to use the telescope to time the eclipse of NN Ser, I used live sessions on the telescope to capture images of NN Ser during an eclipse. The Faulkes Telescope is equipped with a CCD camera. This contains a piece of silicon which detects light through the photoelectric effect, which causes i ...
... In order to use the telescope to time the eclipse of NN Ser, I used live sessions on the telescope to capture images of NN Ser during an eclipse. The Faulkes Telescope is equipped with a CCD camera. This contains a piece of silicon which detects light through the photoelectric effect, which causes i ...
OLEARY_2004_white
... In order to use the telescope to time the eclipse of NN Ser, I used live sessions on the telescope to capture images of NN Ser during an eclipse. The Faulkes Telescope is equipped with a CCD camera. This contains a piece of silicon which detects light through the photoelectric effect, which causes i ...
... In order to use the telescope to time the eclipse of NN Ser, I used live sessions on the telescope to capture images of NN Ser during an eclipse. The Faulkes Telescope is equipped with a CCD camera. This contains a piece of silicon which detects light through the photoelectric effect, which causes i ...
Light year - TeacherWeb
... Light year – the distance light can travel in a year (9.5 trillion km or 5.88 trillion miles / year - that’s 12 “0”s!!!) Just for Interest: Light travels about 300,000 km (186,000 miles) per second The North Star is 431 light years from Earth Our nearest star, Proxima Centauri, is 4.28 light ...
... Light year – the distance light can travel in a year (9.5 trillion km or 5.88 trillion miles / year - that’s 12 “0”s!!!) Just for Interest: Light travels about 300,000 km (186,000 miles) per second The North Star is 431 light years from Earth Our nearest star, Proxima Centauri, is 4.28 light ...
Chapter 10 Workbook
... C. The force of gravity extends beyond the surface of Earth. D. The time a planet takes to revolve around the Sun is directly related to how far away it is from the Sun. 4. Which effect does gravity have on celestial bodies? A. Gravity causes celestial bodies to remain in orbit around larger bodies. ...
... C. The force of gravity extends beyond the surface of Earth. D. The time a planet takes to revolve around the Sun is directly related to how far away it is from the Sun. 4. Which effect does gravity have on celestial bodies? A. Gravity causes celestial bodies to remain in orbit around larger bodies. ...
Final Exam Space Unit Review
... http://missionscience.nasa.gov/ems/emsVideo_01intro.html Don’t forget! Wavelength measures the distance between two similar points on a wave, and frequency is the measure of how many waves pass in a given time period 2) What are stars made of? Use a SPECTROSCOPE! A spectroscope uses visible light in ...
... http://missionscience.nasa.gov/ems/emsVideo_01intro.html Don’t forget! Wavelength measures the distance between two similar points on a wave, and frequency is the measure of how many waves pass in a given time period 2) What are stars made of? Use a SPECTROSCOPE! A spectroscope uses visible light in ...
What is the difference between geocentric and heliocentric theories?
... • Contain very little gas or dust. • Because of little gas, no new stars are forming. • The largest and smallest galaxies are elliptical galaxies. ...
... • Contain very little gas or dust. • Because of little gas, no new stars are forming. • The largest and smallest galaxies are elliptical galaxies. ...
Name: Period : _____ Bulldog Review #9 1. The Milky Wa
... state of technology, what would be the best equipment for these scientists to use to obtain the most detailed data about Saturn’s atmosphere? A. Space probe B. Manned spaceflight C. Telescope from Earth D. Satellite orbiting Earth Use the chart below to answer questions 15 – 17. Stage 1: Gravity pul ...
... state of technology, what would be the best equipment for these scientists to use to obtain the most detailed data about Saturn’s atmosphere? A. Space probe B. Manned spaceflight C. Telescope from Earth D. Satellite orbiting Earth Use the chart below to answer questions 15 – 17. Stage 1: Gravity pul ...
Astronomy - South Kitsap School District
... 817 Pacific Ave, Bremerton, WA 98337 Join us at the Pacific Planetarium on Saturday, May 10th for a FREE day of astronomy activities for everyone! Look through a telescope or watch a planetarium show to see what gets astronomers all excited when they gaze into the universe ...
... 817 Pacific Ave, Bremerton, WA 98337 Join us at the Pacific Planetarium on Saturday, May 10th for a FREE day of astronomy activities for everyone! Look through a telescope or watch a planetarium show to see what gets astronomers all excited when they gaze into the universe ...
The Evolutionary Cycle of Stars
... may briefly outshine its entire host galaxy before fading from view over several weeks or months. The explosion expels much or all of a star's material ...
... may briefly outshine its entire host galaxy before fading from view over several weeks or months. The explosion expels much or all of a star's material ...
Stars
... Stars have different sizes. White dwarf stars are about the size of Earth. Supergiant stars can be wider than 300 million miles. That is more than one thousand times the distance from Earth to the Moon. Stars can be different colors such as blue, yellow, orange, red, white, and black. ...
... Stars have different sizes. White dwarf stars are about the size of Earth. Supergiant stars can be wider than 300 million miles. That is more than one thousand times the distance from Earth to the Moon. Stars can be different colors such as blue, yellow, orange, red, white, and black. ...
Reflecting - Cloudfront.net
... Scintillation or “twinkling” of a star is caused by unstable air refracting the star’s light in different directions. Light is also absorbed and scattered by the atmosphere This means that even an optical telescope works better in Space. Like • Hubble Space Telescope: For “Deep Space” • Kepler Space ...
... Scintillation or “twinkling” of a star is caused by unstable air refracting the star’s light in different directions. Light is also absorbed and scattered by the atmosphere This means that even an optical telescope works better in Space. Like • Hubble Space Telescope: For “Deep Space” • Kepler Space ...
Astronomy work sheet
... Find out the distances of the planets of the Solar System from the Sun. How can you tell from the night sky which planets are closer to the Sun than the Earth? 11. ASTRONOMICAL TERMS What is meant by the following: Galaxy Magnitude Red Shift Black Hole ...
... Find out the distances of the planets of the Solar System from the Sun. How can you tell from the night sky which planets are closer to the Sun than the Earth? 11. ASTRONOMICAL TERMS What is meant by the following: Galaxy Magnitude Red Shift Black Hole ...
the young astronomers newsletter
... Belt at the fringes of our Solar System. It is 3.3 billion miles from Earth and 310 million miles beyond Pluto, clipping along at 14 kilometers per second. It is so far out that speed of light round trip radio messages take nearly ten hours. All systems seem to be working beautifully. As it travels, ...
... Belt at the fringes of our Solar System. It is 3.3 billion miles from Earth and 310 million miles beyond Pluto, clipping along at 14 kilometers per second. It is so far out that speed of light round trip radio messages take nearly ten hours. All systems seem to be working beautifully. As it travels, ...
History of Astronomy
... *** Einstein explained the true nature of gravity. • That it’s not a force but a pathway that a mass takes around more massive objects. This theory was proven correct by the deflection of starlight observed during a 1919 eclipse. c. ...
... *** Einstein explained the true nature of gravity. • That it’s not a force but a pathway that a mass takes around more massive objects. This theory was proven correct by the deflection of starlight observed during a 1919 eclipse. c. ...
Homework #4 Astronomy 101 – Fall 2010 Due November 4, 11 a.m.
... Why not Hubble? Of the more than 200 extrasolar planets discovered, only one likely planet has ever been imaged by the Hubble Space Telescope. What limit’s Hubble’s ability to image planets around other stars? There are two main factors that limit Hubble’s ability to directly image planets orbiting ...
... Why not Hubble? Of the more than 200 extrasolar planets discovered, only one likely planet has ever been imaged by the Hubble Space Telescope. What limit’s Hubble’s ability to image planets around other stars? There are two main factors that limit Hubble’s ability to directly image planets orbiting ...
PHYS 200 - Understanding the Universe
... • grasp how physical principles are applied to understand cosmic objects. • Gain appreciation for science and scientific methods and to realize that progress in the understanding of the Universe is achieved by continual questioning of current knowledge. • Report on: what makes up the solar system, w ...
... • grasp how physical principles are applied to understand cosmic objects. • Gain appreciation for science and scientific methods and to realize that progress in the understanding of the Universe is achieved by continual questioning of current knowledge. • Report on: what makes up the solar system, w ...
Quiz #3 Review
... • recall that comets contain water; they orbit the Sun on very eccentric orbits that extend to the outer solar system where it is cold and therefore they retain their water/ice • asteroids that may have collided with inner planets during the solar system formation likely had little if any water/ice, ...
... • recall that comets contain water; they orbit the Sun on very eccentric orbits that extend to the outer solar system where it is cold and therefore they retain their water/ice • asteroids that may have collided with inner planets during the solar system formation likely had little if any water/ice, ...
dtu7ech03 pt 2 - Fort Thomas Independent Schools
... Angular resolution of ground-based telescopes: a comparison Best resolution: 0.00001” using radio data from telescopes on opposite sides of the Earth 0.001”—VLBA across the US 0.1”—VLA radio wave observatory in New Mexico 0.3” to 0.005”—Keck Observatory, Hawaii ...
... Angular resolution of ground-based telescopes: a comparison Best resolution: 0.00001” using radio data from telescopes on opposite sides of the Earth 0.001”—VLBA across the US 0.1”—VLA radio wave observatory in New Mexico 0.3” to 0.005”—Keck Observatory, Hawaii ...
Jeff Christopher
... If the weather was good all night then I would have a long night of observing. We started off thinking that if we timed it right we could observe maybe two stars a night, but we soon found that their variations we not completely set in stone, so it was better to stick with one variable star and ima ...
... If the weather was good all night then I would have a long night of observing. We started off thinking that if we timed it right we could observe maybe two stars a night, but we soon found that their variations we not completely set in stone, so it was better to stick with one variable star and ima ...
After Dark M S
... What are cosmic rays and how were they discovered? How can particles of light with trillions of times the energy of the light particles from the sun be used to do astronomy and learn about the sources of cosmic rays? HAWC, a cosmic ray observatory currently under construction, will detect and measur ...
... What are cosmic rays and how were they discovered? How can particles of light with trillions of times the energy of the light particles from the sun be used to do astronomy and learn about the sources of cosmic rays? HAWC, a cosmic ray observatory currently under construction, will detect and measur ...
Race to the Moon
... When the sun is at it’s highest point in the sky, we call it…. • Solar Noon ...
... When the sun is at it’s highest point in the sky, we call it…. • Solar Noon ...
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.