Welcome to the Magic Valley Astronomical Society Pomerelle
... Even Grandpa Stan Mayer, who was just hanging around, nights, with more than 65 each night. Many people were waiting for the scopes even prior to sunset, and many kept reported having a good time getting to know members, and even tried to help Tom Gilbertson with the spot scope on coming back to the ...
... Even Grandpa Stan Mayer, who was just hanging around, nights, with more than 65 each night. Many people were waiting for the scopes even prior to sunset, and many kept reported having a good time getting to know members, and even tried to help Tom Gilbertson with the spot scope on coming back to the ...
hubble_refurb
... Joining Mikulski as an advocate for servicing Hubble was NASA's Chief Scientist, physicist John Grunsfeld, who was present at the meeting when O'Keefe announced the cancellation of the mission.[18] A veteran astronaut of four shuttle missions, including two Hubble servicing missions, Grunsfeld had d ...
... Joining Mikulski as an advocate for servicing Hubble was NASA's Chief Scientist, physicist John Grunsfeld, who was present at the meeting when O'Keefe announced the cancellation of the mission.[18] A veteran astronaut of four shuttle missions, including two Hubble servicing missions, Grunsfeld had d ...
Demonstration of Adaptive Optics in a
... sensor can be used to correct for distortions caused by turbulence in the Earth’s atmosphere. Adaptive optics (AO) systems are currently implemented at a number of national astronomical observatories, including the W. M. Keck Observatory, Gemini, and Subaru, and is a key design component for the nex ...
... sensor can be used to correct for distortions caused by turbulence in the Earth’s atmosphere. Adaptive optics (AO) systems are currently implemented at a number of national astronomical observatories, including the W. M. Keck Observatory, Gemini, and Subaru, and is a key design component for the nex ...
What is Astronomy? - Wayne State University Physics and Astronomy
... •Astronomers use physics and other sciences to interpret the data they collect. •Astronomers are interested in the evolution of our universe and how it was created. They want to understand the objects in our Solar System and elsewhere in the cosmos, and how these objects and phenomena will change ov ...
... •Astronomers use physics and other sciences to interpret the data they collect. •Astronomers are interested in the evolution of our universe and how it was created. They want to understand the objects in our Solar System and elsewhere in the cosmos, and how these objects and phenomena will change ov ...
Gaia Fact Sheet
... data is now widely used by the entire community of professional astronomers. ...
... data is now widely used by the entire community of professional astronomers. ...
Deep-sky-object hunter
... The base goes together with only a supplied Allen wrench, and assembly is intuitive if you’ve ever been around a Dobsonian mount. If not, the instructions will guide you through the assembly process. The OTA comes in two parts, the primary mirror box and the secondary mirror and focuser cage. Three ...
... The base goes together with only a supplied Allen wrench, and assembly is intuitive if you’ve ever been around a Dobsonian mount. If not, the instructions will guide you through the assembly process. The OTA comes in two parts, the primary mirror box and the secondary mirror and focuser cage. Three ...
Science Focus 8 Light and Optical Systems Topic 5 Topic 5
... The lens in a refracting telescope and the mirror in a reflecting telescope collect as much light as possible from distant objects. These collectors then focus the light into an image. The further away the image is from the lens, or the mirror, the greater the magnification. For the greatest magnifi ...
... The lens in a refracting telescope and the mirror in a reflecting telescope collect as much light as possible from distant objects. These collectors then focus the light into an image. The further away the image is from the lens, or the mirror, the greater the magnification. For the greatest magnifi ...
virtual telescope.
... Virtual telescope protypes at GAVO Here we show examples of existing web applications that illustrate the concept of the virtual telescope. By modeling the relevant aspects of the real observational configuration, including sources, possible absorbing/emitting/lensing foregrounds as well as the inst ...
... Virtual telescope protypes at GAVO Here we show examples of existing web applications that illustrate the concept of the virtual telescope. By modeling the relevant aspects of the real observational configuration, including sources, possible absorbing/emitting/lensing foregrounds as well as the inst ...
A Unified Domain Model for Astronomy
... Virtual telescope protypes at GAVO Here we show examples of existing web applications that illustrate the concept of the virtual telescope. By modeling the relevant aspects of the real observational configuration, including sources, possible absorbing/emitting/lensing foregrounds as well as the inst ...
... Virtual telescope protypes at GAVO Here we show examples of existing web applications that illustrate the concept of the virtual telescope. By modeling the relevant aspects of the real observational configuration, including sources, possible absorbing/emitting/lensing foregrounds as well as the inst ...
The magnitude scale
... times fainter again, i.e. 10,000 times fainter than one at the naked eye limit, and so on. ...
... times fainter again, i.e. 10,000 times fainter than one at the naked eye limit, and so on. ...
Two Small Pieces of Glass: The Amazing Telescope
... two small pieces of glass -- to the launch of NASA’s Hubble Space Telescope and the future of astronomy. It explores the wonder and discovery made by astronomers throughout the last 400 years. Activities: Choosing the location for a telescope, the speed of light, creating a model of the Moon. LEARNI ...
... two small pieces of glass -- to the launch of NASA’s Hubble Space Telescope and the future of astronomy. It explores the wonder and discovery made by astronomers throughout the last 400 years. Activities: Choosing the location for a telescope, the speed of light, creating a model of the Moon. LEARNI ...
Brownies worksheet
... Jodrell Bank Discovery Centre Brownies Planet Path Questions! (Page 2) Now go further towards the whispering dishes. Find Saturn and stand on it. Look back to the Earth! The Planet Path shows the distances between the planets ‘to scale’. If the planets were in the positions shown on the Planet Path ...
... Jodrell Bank Discovery Centre Brownies Planet Path Questions! (Page 2) Now go further towards the whispering dishes. Find Saturn and stand on it. Look back to the Earth! The Planet Path shows the distances between the planets ‘to scale’. If the planets were in the positions shown on the Planet Path ...
Broad Sheet 7 - Museum of the History of Science
... the night sky. The telescopic needs of the former were met by a refractor of relatively modest aperture, equipped as a sight, whereas a reflector suited the latter, since the larger aperture possible with a mirror was good for admiring detail in the solar system or wondering at fainter and farther o ...
... the night sky. The telescopic needs of the former were met by a refractor of relatively modest aperture, equipped as a sight, whereas a reflector suited the latter, since the larger aperture possible with a mirror was good for admiring detail in the solar system or wondering at fainter and farther o ...
telescope
... mirror to gather and focus light from distant objects • When light enters a reflecting telescope, the light is reflected by a large curved mirror to a second mirror. The second mirror reflects the light to the eyepiece, where the image is magnified and focused. • Mirrors in reflecting telescopes can ...
... mirror to gather and focus light from distant objects • When light enters a reflecting telescope, the light is reflected by a large curved mirror to a second mirror. The second mirror reflects the light to the eyepiece, where the image is magnified and focused. • Mirrors in reflecting telescopes can ...
Teaching STEM through Big Telescopes
... www.nationalstemcentre.org.uk/elibrary/resource/6114/the-esa-esoastronomy-exercise-series Galaxies. This resource has been devised by The Royal Observatory Edinburgh with the Institute of Physics Scotland, to inspire secondary science classes. They are mainly used by students aged 11-14 years but ca ...
... www.nationalstemcentre.org.uk/elibrary/resource/6114/the-esa-esoastronomy-exercise-series Galaxies. This resource has been devised by The Royal Observatory Edinburgh with the Institute of Physics Scotland, to inspire secondary science classes. They are mainly used by students aged 11-14 years but ca ...
Wave: a disturbance which carries energy through a material or
... Transmission through earth’s atmosphere depends upon wavelength [Fig 6-29] Light Pollution [figure 6.30] Optical Observatories [fig 6.32(Kitt Peak), fig 6.33 (Chile) fig 6.34 Hawaii] Radio Telescopes: larger wavelengths = more resolution problems Large Dishes (arecibo [fig 6.40]) increased resolutio ...
... Transmission through earth’s atmosphere depends upon wavelength [Fig 6-29] Light Pollution [figure 6.30] Optical Observatories [fig 6.32(Kitt Peak), fig 6.33 (Chile) fig 6.34 Hawaii] Radio Telescopes: larger wavelengths = more resolution problems Large Dishes (arecibo [fig 6.40]) increased resolutio ...
![( ) Microscope [Reading Hecht 5.7.3, 5.7.5] Simple microscope (magnifier)](http://s1.studyres.com/store/data/008906619_1-713a6abc204beda0534960f18d7015c8-300x300.png)
( ) Microscope [Reading Hecht 5.7.3, 5.7.5] Simple microscope (magnifier)
... Older microscope objectives (before 1980) were designed to form an image at a given distance (the tube length) behind the objective flange. This distance varied between 160 mm and 210 mm depending on the manufacturer and the application. At the proper tube length, the objectives formed images at the ...
... Older microscope objectives (before 1980) were designed to form an image at a given distance (the tube length) behind the objective flange. This distance varied between 160 mm and 210 mm depending on the manufacturer and the application. At the proper tube length, the objectives formed images at the ...
Buying Your First Telescope - Naples Free-Net
... goes up - way up – from there. Still it’s possible to get a decent sized dobsonian reflector without electronics that will give you a lifetime of magnificent viewing for well under $1,000. Electronics and/or sophisticated mounts make the telescope cost sharply higher. Cost increases still more if yo ...
... goes up - way up – from there. Still it’s possible to get a decent sized dobsonian reflector without electronics that will give you a lifetime of magnificent viewing for well under $1,000. Electronics and/or sophisticated mounts make the telescope cost sharply higher. Cost increases still more if yo ...
Document
... • Signals from these arrays of widely-separated telescopes are added together to create images with very high resolution. • In fact, the resolution is equivalent to that of a single telescope with an aperture as large as the separation between telescopes in the array! ...
... • Signals from these arrays of widely-separated telescopes are added together to create images with very high resolution. • In fact, the resolution is equivalent to that of a single telescope with an aperture as large as the separation between telescopes in the array! ...
( ) Microscope Simple microscope (magnifier)
... Older microscope objectives (before 1980) were designed to form an image at a given distance (the tube length) behind the objective flange. This distance varied between 160 mm and 210 mm depending on the manufacturer and the application. At the proper tube length, the objectives formed images at the ...
... Older microscope objectives (before 1980) were designed to form an image at a given distance (the tube length) behind the objective flange. This distance varied between 160 mm and 210 mm depending on the manufacturer and the application. At the proper tube length, the objectives formed images at the ...
Infrared Spectroscopy of comet Hale-Bopp
... • As expected large abundances of H2O an CO was observed. As well as traces of C2H6, C2H2, CH4 and HCN. • No significant differences of physical properties or chemical composition from P/Halley comet. • Molecular production rates dependence on heliocentric distance provide understanding of physical ...
... • As expected large abundances of H2O an CO was observed. As well as traces of C2H6, C2H2, CH4 and HCN. • No significant differences of physical properties or chemical composition from P/Halley comet. • Molecular production rates dependence on heliocentric distance provide understanding of physical ...
Final Exam Space Unit Review
... b) liquid: more complicated, more efficient because can control amount of fuel entering combustion chamber so can stop or throttle. They have a higher exhaust velocity than solid fuels. Check on this c) Physics: For every reaction there is an equal and opposite reaction d) gravitational assist “slin ...
... b) liquid: more complicated, more efficient because can control amount of fuel entering combustion chamber so can stop or throttle. They have a higher exhaust velocity than solid fuels. Check on this c) Physics: For every reaction there is an equal and opposite reaction d) gravitational assist “slin ...
James Webb Space Telescope
The James Webb Space Telescope (JWST), previously known as Next Generation Space Telescope (NGST), is a space observatory under construction and scheduled to launch in October 2018. The JWST will offer unprecedented resolution and sensitivity from long-wavelength visible to the mid-infrared, and is a successor instrument to the Hubble Space Telescope and the Spitzer Space Telescope. The telescope features a segmented 6.5-meter (21 ft) diameter primary mirror and will be located near the Earth–Sun L2 point. A large sunshield will keep its mirror and four science instruments below 50 K (−220 °C; −370 °F).JWST's capabilities will enable a broad range of investigations across the fields of astronomy and cosmology. One particular goal involves observing some of the most distant objects in the Universe, beyond the reach of current ground and space based instruments. This includes the very first stars, the epoch of reionization, and the formation of the first galaxies. Another goal is understanding the formation of stars and planets. This will include imaging molecular clouds and star-forming clusters, studying the debris disks around stars, direct imaging of planets, and spectroscopic examination of planetary transits.In gestation since 1996, the project represents an international collaboration of about 17 countries led by NASA, and with significant contributions from the European Space Agency and the Canadian Space Agency. It is named after James E. Webb, the second administrator of NASA, who played an integral role in the Apollo program.The JWST has a history of major cost overruns and delays. The first realistic budget estimates were that the observatory would cost $1.6 billion and launch in 2011. NASA has now scheduled the telescope for a 2018 launch. In 2011, the United States House of Representatives voted to terminate funding, after about $3 billion had been spent and 75 percent of its hardware was in production. Funding was restored in compromise legislation with the US Senate, and spending on the program was capped at $8 billion. As of December 2014, the telescope remained on schedule and within budget, but at risk of further delays.