Optics and Telescopes
... Spectroscopy is one of the most important parts of observational astronomy. Spectral observations can tell us the temperature, chemical composition, and motion of remote celestial objects. ...
... Spectroscopy is one of the most important parts of observational astronomy. Spectral observations can tell us the temperature, chemical composition, and motion of remote celestial objects. ...
Document
... 1. A Newtonian focus reflecting telescope has a plane mirror mounted along the axis of the telescope so that the mirror intercepts the light from the objective mirror and reflects it to the side. 2. A Cassegrain focus reflecting telescope has a secondary convex mirror that reflects the light back th ...
... 1. A Newtonian focus reflecting telescope has a plane mirror mounted along the axis of the telescope so that the mirror intercepts the light from the objective mirror and reflects it to the side. 2. A Cassegrain focus reflecting telescope has a secondary convex mirror that reflects the light back th ...
1B11 Foundations of Astronomy Star names and magnitudes
... Telescopes in the ultraviolet and infra-red are similar in concept to optical telescopes, but are orbiting space observatories – launched beyond the Earth’s atmosphere which is opaque at these wavelengths. Conventional CCDs are not sensitive, particularly at wavelengths longer than 1mm, so different ...
... Telescopes in the ultraviolet and infra-red are similar in concept to optical telescopes, but are orbiting space observatories – launched beyond the Earth’s atmosphere which is opaque at these wavelengths. Conventional CCDs are not sensitive, particularly at wavelengths longer than 1mm, so different ...
Telescopes and instruments
... Telescopes in the ultraviolet and infra-red are similar in concept to optical telescopes, but are orbiting space observatories – launched beyond the Earth’s atmosphere which is opaque at these wavelengths. Conventional CCDs are not sensitive, particularly at wavelengths longer than 1mm, so different ...
... Telescopes in the ultraviolet and infra-red are similar in concept to optical telescopes, but are orbiting space observatories – launched beyond the Earth’s atmosphere which is opaque at these wavelengths. Conventional CCDs are not sensitive, particularly at wavelengths longer than 1mm, so different ...
of light
... One such array is called the Very Large Baseline Array (VLBA): it consists of ten radio telescopes which reach all the way from Hawaii to Puerto Rico: nearly a third of the way around the world! By putting a radio telescope in orbit around the Earth, radio astronomers could make images as if they ha ...
... One such array is called the Very Large Baseline Array (VLBA): it consists of ten radio telescopes which reach all the way from Hawaii to Puerto Rico: nearly a third of the way around the world! By putting a radio telescope in orbit around the Earth, radio astronomers could make images as if they ha ...
Tools of Astronomy - Indiana University Astronomy
... meter diameter • Located at Kitt Peak, Arizona • Built in 1995 • IU has a share ...
... meter diameter • Located at Kitt Peak, Arizona • Built in 1995 • IU has a share ...
January
... The GMT is slated for completion in 2016 at a site in Northern Chile. Viewing conditions in Chile, such as at Carnegie's Las Campanas Observatory, are some of the best in the world. The GMT will have ten times the resolution of the Hubble Space Telescope. With its powerful resolution and enormous co ...
... The GMT is slated for completion in 2016 at a site in Northern Chile. Viewing conditions in Chile, such as at Carnegie's Las Campanas Observatory, are some of the best in the world. The GMT will have ten times the resolution of the Hubble Space Telescope. With its powerful resolution and enormous co ...
The Telescope and the Microscope Lab
... Telescope Mtheo = 3.45 Mexp = 4 % Error % diff = 10.1 % ...
... Telescope Mtheo = 3.45 Mexp = 4 % Error % diff = 10.1 % ...
Observatory, Domes, and Telescopes
... Observatory and operate as a system. These facilities extend across two mountaintops: Mt. Locke and Mt. Fowlkes. Specific characteristics of observatory, dome, a n d telescope that students may show in their drawings: Dome: Encloses the telescope. HJS 2.7-m and Struve 2.1-m telescope domes have curv ...
... Observatory and operate as a system. These facilities extend across two mountaintops: Mt. Locke and Mt. Fowlkes. Specific characteristics of observatory, dome, a n d telescope that students may show in their drawings: Dome: Encloses the telescope. HJS 2.7-m and Struve 2.1-m telescope domes have curv ...
Presentation: Light and Telescopes
... All of these regions can be used in astronomy to measure objects in the universe. Different methods are needed to detect different wavelengths of radiation. Only certain parts of the E-M spectrum can penetrate the Earth’s atmosphere. ...
... All of these regions can be used in astronomy to measure objects in the universe. Different methods are needed to detect different wavelengths of radiation. Only certain parts of the E-M spectrum can penetrate the Earth’s atmosphere. ...
6 Very High Energy Gamma Ray Astronomy with CTA - UZH
... Max Plank Institute for Nuclear Physics (MPI-K) in Heidelberg, Germany have shown that adequate instrumental and timing resolution can be achieved by using a system that samples at a rate of 250 MS/s. A telescope array of such digitizers is feasible, and is currently being prototyped. A prototype mo ...
... Max Plank Institute for Nuclear Physics (MPI-K) in Heidelberg, Germany have shown that adequate instrumental and timing resolution can be achieved by using a system that samples at a rate of 250 MS/s. A telescope array of such digitizers is feasible, and is currently being prototyped. A prototype mo ...
![Collecting Area [km 2 ]](http://s1.studyres.com/store/data/005251749_1-ac6dff2cb85965aa98ca71572274094f-300x300.png)
Collecting Area [km 2 ]
... (now also possible >20keV, hence NuSTAR) Low energy x-ray detectors could be built from silicon -> CCDs Low energy single photon resolution became sub arcsec ...
... (now also possible >20keV, hence NuSTAR) Low energy x-ray detectors could be built from silicon -> CCDs Low energy single photon resolution became sub arcsec ...
Telescope Lab - Harvard-Smithsonian Center for Astrophysics
... Taking an image. Explain to students that they will control the robotic telescope remotely. They will select the target star and several observing times. At night, the telescope will automatically point to ...
... Taking an image. Explain to students that they will control the robotic telescope remotely. They will select the target star and several observing times. At night, the telescope will automatically point to ...
The definition of a microscope: An instrument for viewing objects that
... the naked eye. Circa 1284 - Italian, Salvino D'Armate is credited with inventing the first wearable eye glasses. Hans Lippershey (ca. 1570-1619), a German-Dutch lens grinder and spectacle (glasses) maker, is generally credited with inventing the telescope. This is because in 1608 Lippsershey became ...
... the naked eye. Circa 1284 - Italian, Salvino D'Armate is credited with inventing the first wearable eye glasses. Hans Lippershey (ca. 1570-1619), a German-Dutch lens grinder and spectacle (glasses) maker, is generally credited with inventing the telescope. This is because in 1608 Lippsershey became ...
The Dragonfly Telephoto Array
... images, well below our detection limit. A summary of the reby the reflected light. The size of the two largest reflections corflecting surfaces and the brightness of their reflections is prerespond to a reflecting surface 3.6 cm away from the CCD, sented in Table 1. which matches the position of the ...
... images, well below our detection limit. A summary of the reby the reflected light. The size of the two largest reflections corflecting surfaces and the brightness of their reflections is prerespond to a reflecting surface 3.6 cm away from the CCD, sented in Table 1. which matches the position of the ...
Galileo, Brahe, and Kepler - Pennsylvania State University
... SKA will be an array of thousands of radio dishes with a total collecting area of 1 km2 and a baseline of 3000 km. It will be built in either Australia or Africa and should begin operations in 2020. SKA will offer both sharp images (<0.1”) and a huge field of view (1 deg), as well as 100x the sensit ...
... SKA will be an array of thousands of radio dishes with a total collecting area of 1 km2 and a baseline of 3000 km. It will be built in either Australia or Africa and should begin operations in 2020. SKA will offer both sharp images (<0.1”) and a huge field of view (1 deg), as well as 100x the sensit ...
Make your own Telescope
... 1. Add the lengths of the two lenses. Your cardboard tubes will need to be able to extend to at least this length. 2. Make a cardboard tube 10cm in length from the black cardboard. Use blu-tac to secure the largest convex lens in the end of the tube. 3. To calculate the length for the second cardboa ...
... 1. Add the lengths of the two lenses. Your cardboard tubes will need to be able to extend to at least this length. 2. Make a cardboard tube 10cm in length from the black cardboard. Use blu-tac to secure the largest convex lens in the end of the tube. 3. To calculate the length for the second cardboa ...
AMSAT 1m Dish - Del Mar North
... means Earth-to-Space (uplink) direction only means Space-to-Earth (downlink) direction only * the 9 cm satellite band is only available in regions 2 & 3 ...
... means Earth-to-Space (uplink) direction only means Space-to-Earth (downlink) direction only * the 9 cm satellite band is only available in regions 2 & 3 ...
$doc.title
... • Thermally generated electrons are indistinguishable from photogenerated electrons Dark Current keep the CCD cold! • Silicon is transparent to photons with E < 1.26eV (λ ≈ 1.05 µm) Red Cutoff! Need a different type of detector for IR … ...
... • Thermally generated electrons are indistinguishable from photogenerated electrons Dark Current keep the CCD cold! • Silicon is transparent to photons with E < 1.26eV (λ ≈ 1.05 µm) Red Cutoff! Need a different type of detector for IR … ...
Quiz # 3
... 8. If one observatory site is described as having better “seeing” than another observatory site, what is it that is better at the first site? A) The sky is more transparent and there is less haze in the atmosphere at that site, providing brighter and sharper images. B) The winds are lighter at the ...
... 8. If one observatory site is described as having better “seeing” than another observatory site, what is it that is better at the first site? A) The sky is more transparent and there is less haze in the atmosphere at that site, providing brighter and sharper images. B) The winds are lighter at the ...
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 ...
Proposal memo example - University of Portland
... size. Weight and ease of set-up and take-down are also important criteria. A modified truss tube design best meets the criteria. It will use two tubes and a series of strings to hold the secondary holder in place. This will be similar to designs described in various web pages [2, 3]. This design off ...
... size. Weight and ease of set-up and take-down are also important criteria. A modified truss tube design best meets the criteria. It will use two tubes and a series of strings to hold the secondary holder in place. This will be similar to designs described in various web pages [2, 3]. This design off ...
Radio Telescopes
... • Used to study invisible radiation, light we don’t see. • The entire electromagnetic spectrum is used because different types of radiation reveal different clues about the objects being studied. • Examples of light we don’s see. It is detected as heat/radiation: radio waves, x-rays, microwaves, gam ...
... • Used to study invisible radiation, light we don’t see. • The entire electromagnetic spectrum is used because different types of radiation reveal different clues about the objects being studied. • Examples of light we don’s see. It is detected as heat/radiation: radio waves, x-rays, microwaves, gam ...
Allen Telescope Array
The Allen Telescope Array (ATA), formerly known as the One Hectare Telescope (1hT) is a radio telescope array dedicated to astronomical observations and a simultaneous Search for Extraterrestrial Intelligence (SETI). The array is situated at the Hat Creek Radio Observatory, 290 miles (470 km) northeast of San Francisco, California.Originally developed as a joint effort between the SETI Institute and the Radio Astronomy Laboratory (RAL) at the University of California, Berkeley (UC Berkley) with funds obtained from an initial US$11.5 million donation by the Paul G. Allen Family Foundation, the project completed the first phase of construction and become operational on 11 October 2007 with 42 antennas (ATA-42), after Paul Allen (co-founder of Microsoft) pledged an additional $13.5 million to support the construction of the first and second phases.Though overall Allen has contributed more than $30 million to the project, the project has not succeeded in building the 350 six metre (19.7 feet) dishes originally conceived, and suffered an operational hiatus due to funding shortfalls between April and August 2011. Subsequently, UC Berkeley exited the project, completing divestment in April 2012. The facility is now managed by SRI International (formerly Stanford Research Institute), an independent, nonprofit research institute.In August 2014 the installation was threatened by a forest fire in the area and was briefly forced to shut down, but ultimately emerged largely unscathed.