Lab 6 - College of San Mateo
... previous step, place the image precisely on the intersection of the crosshairs. Read THE SAME window as in the previous step. The difference between the two readings should be 120° ± 30'. If it is not, recheck both readings. (If the scale passed through zero while the prism was rotated, add 360° to ...
... previous step, place the image precisely on the intersection of the crosshairs. Read THE SAME window as in the previous step. The difference between the two readings should be 120° ± 30'. If it is not, recheck both readings. (If the scale passed through zero while the prism was rotated, add 360° to ...
Stars - Open Court Resources.com
... and dust called nebula. The article I read in the science magazine was about a nebula, a large cloud of gas and dust in outer space. Definition – glowing clouds of gas and dust amidst the clouds. ...
... and dust called nebula. The article I read in the science magazine was about a nebula, a large cloud of gas and dust in outer space. Definition – glowing clouds of gas and dust amidst the clouds. ...
May 2013 - Faculty
... highest and Jupiter being the lowest). This grouping takes place in bright twilight, but should still be easily visible since all three planets are very bright. The other side of the night sky prior to midnight contains the planet Saturn. Saturn is at opposition on April 28th, and as such, will rise ...
... highest and Jupiter being the lowest). This grouping takes place in bright twilight, but should still be easily visible since all three planets are very bright. The other side of the night sky prior to midnight contains the planet Saturn. Saturn is at opposition on April 28th, and as such, will rise ...
template
... SPICA is a JAXA led mission scheduled for launch by 2018 (Phase A). Medium and far IR observatory (5 – 210 um), with sky background limited sensitivity via a cryogenically cooled telescope (3.5 m diameter, T < 6K). Launcher vehicle is JAXA’s HII-B. Large halo orbit at SE-L2 (P ~ 180 days). Nominal m ...
... SPICA is a JAXA led mission scheduled for launch by 2018 (Phase A). Medium and far IR observatory (5 – 210 um), with sky background limited sensitivity via a cryogenically cooled telescope (3.5 m diameter, T < 6K). Launcher vehicle is JAXA’s HII-B. Large halo orbit at SE-L2 (P ~ 180 days). Nominal m ...
What is Ocean Color Data? - USF College of Marine Science
... Ultraviolet observatories Right now there are no dedicated ultraviolet observatories in orbit. The Hubble Space Telescope can perform a great deal of observing at ultraviolet wavelengths, but it has a very fairly small field of view. Water vapor in the atmosphere ...
... Ultraviolet observatories Right now there are no dedicated ultraviolet observatories in orbit. The Hubble Space Telescope can perform a great deal of observing at ultraviolet wavelengths, but it has a very fairly small field of view. Water vapor in the atmosphere ...
Custom Solutions Catalog
... All of the Spiral Galilean Telescopes can be fitted in either the full diameter on center position or in the bioptic position mounted as high as possible above the geometric center of the frame. As the diameter of the eye pieces of the Spiral Galilean Telescopes differ, height placement of the syste ...
... All of the Spiral Galilean Telescopes can be fitted in either the full diameter on center position or in the bioptic position mounted as high as possible above the geometric center of the frame. As the diameter of the eye pieces of the Spiral Galilean Telescopes differ, height placement of the syste ...
Some Applications of Lenses
... Soon after they were in use, humans made more progress in medical science than had been made in the thousands of years prior to their invention. Microscopes gave investigators the tools to observe and make inferences about what they saw. It became possible to see that organisms were made up of small ...
... Soon after they were in use, humans made more progress in medical science than had been made in the thousands of years prior to their invention. Microscopes gave investigators the tools to observe and make inferences about what they saw. It became possible to see that organisms were made up of small ...
The New Worlds Observer
... as the completeness for that star2 (Fig. 3). If there is one planet per HZ on average (HZ=1), then the completeness is the expected number of HZ planets detected. We sum the completeness for each observed star to get the total completeness for the mission. We created sample mission schedules to det ...
... as the completeness for that star2 (Fig. 3). If there is one planet per HZ on average (HZ=1), then the completeness is the expected number of HZ planets detected. We sum the completeness for each observed star to get the total completeness for the mission. We created sample mission schedules to det ...
Day Laboratory Exercise #3: Optics and Telescopes
... With the eyepiece lens removed, but the secondary mirror in place, measure the focal length of the primary mirror by projecting an image onto a piece of paper held to the side, near the secondary mirror, and moving the paper until the image is in focus. Measure the distance from the paper to the cen ...
... With the eyepiece lens removed, but the secondary mirror in place, measure the focal length of the primary mirror by projecting an image onto a piece of paper held to the side, near the secondary mirror, and moving the paper until the image is in focus. Measure the distance from the paper to the cen ...
Poster
... large-scale response of detector (L-flat): f(l), f(x,y) All of these contributions need to be measured at component level and built into a physical/optical instrument model. Once NIRSpec is assembled, they cannot be measured individually. However, once a shutter has been specified, all of them are ...
... large-scale response of detector (L-flat): f(l), f(x,y) All of these contributions need to be measured at component level and built into a physical/optical instrument model. Once NIRSpec is assembled, they cannot be measured individually. However, once a shutter has been specified, all of them are ...
Technical Challenges and Parameters for a Future Design Simon Swordy University of Chicago
... • Non-spherical mirror manufacture will most likely be required. Exploration of cost effective replication schemes is needed. • High quantum efficiency devices are very attractive. Doubling existing bialkali QE to ~50% would reduce the cost of the telescope by a significant amount (x2-3) and might u ...
... • Non-spherical mirror manufacture will most likely be required. Exploration of cost effective replication schemes is needed. • High quantum efficiency devices are very attractive. Doubling existing bialkali QE to ~50% would reduce the cost of the telescope by a significant amount (x2-3) and might u ...
equipment introduction
... The last task – Don’t forget this!! Watch any one of the above objects for 2 minutes in the eyepiece, and record what happens in the “notes.” Highlight (with color, borders, etc.) your observation to make it easy for me to find when grading. Your grade for this lab Each sketch except #5 (Gomeisa or ...
... The last task – Don’t forget this!! Watch any one of the above objects for 2 minutes in the eyepiece, and record what happens in the “notes.” Highlight (with color, borders, etc.) your observation to make it easy for me to find when grading. Your grade for this lab Each sketch except #5 (Gomeisa or ...
The LAMA prototype telescope - UBC
... layer that is as thin as possible to rapidly damp surface waves1. The high surface tension mercury combined with mercury’s inability to wet most surfaces makes it difficult to form a large continuous surface, particularly if the layer is thin. The 6.0 meter Large Zenith Telescope and the smaller liq ...
... layer that is as thin as possible to rapidly damp surface waves1. The high surface tension mercury combined with mercury’s inability to wet most surfaces makes it difficult to form a large continuous surface, particularly if the layer is thin. The 6.0 meter Large Zenith Telescope and the smaller liq ...
... With the eyepiece lens removed, but the secondary mirror in place, measure the focal length of the primary mirror by projecting an image onto a piece of paper held to the side, near the secondary mirror, and moving the paper until the image is in focus. Measure the distance from the paper to the cen ...
chris - ESA Earth Online
... Smile is curvature and tilt of the image of a straight entrance slit, which introduces a nonuniformity in the wavelengths defined by each row of detector elements. Frown is a variation in tilt of the spectra associated with each point on ground, introducing errors in spatial registration of spectral ...
... Smile is curvature and tilt of the image of a straight entrance slit, which introduces a nonuniformity in the wavelengths defined by each row of detector elements. Frown is a variation in tilt of the spectra associated with each point on ground, introducing errors in spatial registration of spectral ...
What`s Up? - Santiago Canyon College
... times greater than our Sun’s mass and whose radius is 936 times greater than our sun. If Betelgeuse were in the position our Sun is in, it would engulf the orbit of the planets up through Mars. It is anticipated that Betelgeuse will go super nova within the next 1000 years. South of Orion’s Belt (ag ...
... times greater than our Sun’s mass and whose radius is 936 times greater than our sun. If Betelgeuse were in the position our Sun is in, it would engulf the orbit of the planets up through Mars. It is anticipated that Betelgeuse will go super nova within the next 1000 years. South of Orion’s Belt (ag ...
