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Chapter 5
Chapter 5

... 5.2 Telescope Size Resolving power: When better, can distinguish objects that are closer together Resolution is proportional to wavelength and inversely proportional to telescope size—bigger is better! © 2011 Pearson Education, Inc. ...
Hubble Error: Time, Money and Millionths of an inch
Hubble Error: Time, Money and Millionths of an inch

... had only a few days left for the final adjustment: the distance between the lower of the mirrors and the lens. Special rods had been manufactured to measure the spaces. The rods were made of Invar, a material that doesn’t expand or contract in heat or cold. They had been measured and cut, then shipp ...
Isaac Newton Test - Garden of Praise
Isaac Newton Test - Garden of Praise

Scientific Strategic Plan 2009
Scientific Strategic Plan 2009

... balanced with a steady regard for the many smaller but no less vital elements that in combination maintain Keck as a leading astronomical observatory ...
A Teacher`s Guide
A Teacher`s Guide

... a piece of paper to cover up the parts of the sentences that come after the ellipses. One at a time, have your students try to guess the end of each of the sentences and then when they are close enough to the right answer, uncover the sentence. 3. Tell the students that satellites are sent into spac ...
www.aavso.org
www.aavso.org

... Think of the Intensity as the amount of photons emitted over time. The intensity is what is measured for photometry. ...
Topic 2 - Holy Cross Collegiate
Topic 2 - Holy Cross Collegiate

... around the end of the smaller diameter tube until you get a snug fit. You should be able to slide the smaller diameter tube in and out of the larger tube. Adjust the distance between ...
Radio Telescopes
Radio Telescopes

... study what lies beyond Earth's atmosphere. For example, the twin Keck reflecting telescopes, shown in Figure 4, have segmented mirrors 10 in wide. Until 2000, these mirrors were the largest reflectors ever used. To cope with the difficulty of building such huge mirrors, the Keck telescope mirrors ar ...
thin silicon carbide coating of the primary mirror of vuv imaging
thin silicon carbide coating of the primary mirror of vuv imaging

... Figure 3: The transmission, reflectance, and absorption of the solar spectral irradiance of the three SiC mirror samples. The spectral curves were calculated from the measured photometric properties using the solar irradiance from the „Solar 2000 Model“ spectrum of January 2000. The upper right corn ...
What is a galaxy - University of Melbourne
What is a galaxy - University of Melbourne

star pattern identification : application to the precise attitude
star pattern identification : application to the precise attitude

... by the Russian Space Agency in cooperation with the international scientific community which are dedicated to magnetospheric research. This spacecraft is subject to the effects of energy exchange between the flexible booms and the main body. This energy pumping over induced a rise of the nutation an ...
Unit 5 – Space Exploration - Buck Mountain Central School
Unit 5 – Space Exploration - Buck Mountain Central School

... An innovation for ground-based optical reflecting telescopes is the use of segmented mirrors (a segmented-mirror telescope uses several lightweight-segments to build one large mirror). Interferometry: Combining Telescopes for Greater Power. The technique of using a number of telescopes in combinatio ...
L`imageur de Fresnel - Laboratoire Astrophysique de Toulouse
L`imageur de Fresnel - Laboratoire Astrophysique de Toulouse

tut44 Making A Mirror Grinding Tool
tut44 Making A Mirror Grinding Tool

... huge. Today, with the low-cost imported telescopes, making your own telescope may not save you any money, but you definitely can build your own telescope, and almost any homemade telescope will have higher quality optics than the imported equivalent scope you can buy. The image below was taken using ...
Downloadable Full Text
Downloadable Full Text

Monsalve - Conference
Monsalve - Conference

... • Main science objective is to improve characterization of Emode polarization and detect the difficult B-mode polarization • Two phases are planned. Phase-I is ongoing, started in August 2008. Phase II is planned to start in 2012, in a larger scale, improving the techniques learned during phase-I ...
AAS_LongBeach_Pasach.. - Science Center
AAS_LongBeach_Pasach.. - Science Center

... moving parts that go into any transit observation, for planets in our solar system or outside it. Only about 90% of the dips in stellar brightness observed with the Kepler spacecraft are actually from exoplanet transits, so it is especially important to understand all the workings of transits. The c ...
Results from the search for tidal disruption flares in the GALEX Deep
Results from the search for tidal disruption flares in the GALEX Deep

... • Seyfert nucleus in it inner 0.”1 was previously masked by H II regions in ground-based spectra • The Chandra upper-limit on the nuclear X-ray luminosity is consistent with the predicted Lx from L(H) for LLAGNs, of ~ 9 x 1038 ergs s-1. ...
Make your own telescope
Make your own telescope

Supernova Stalking - Susanna Kumlien Reportage
Supernova Stalking - Susanna Kumlien Reportage

03 Telescopes - Physics and Astronomy
03 Telescopes - Physics and Astronomy

... A. it can better focus x-ray images. B. in orbit, it can operate close to its diffraction limit at visible wavelengths. C. it is larger than any Earth-based scopes. ...
Document
Document

... identify and subtract the signal in its detection band from every merging neutron star and black hole binary in the universe. It will also extend LISA’s scientific program of measuring wavesfrom the merging of intermediate-mass black holes at any redshift, and will refine the mapping of space-time a ...
EUS REVIEW TO PPARC JAN 2004 (Harrison)
EUS REVIEW TO PPARC JAN 2004 (Harrison)

...  Solar EUV spectrometer – to identify & analyse emission lines from trace elements in the solar atmosphere, providing plasma diagnostic information for many applications – it is a general purpose solar plasma diagnostic tool!  Builds on the highly successful RAL-led SOHO/CDS – just completed its 8 ...
lab10 - University of Puget Sound
lab10 - University of Puget Sound

... formed by the objective but becomes the object for the eyepiece). All of the other rays of light that leave the tip of the arrow and go through the lens also converge of the tip of the intermediate image. Pretty amazing! In a microscope the eyepiece is used as a magnifying glass to form a final imag ...
Extreme Optics and the Search for Earth-Like Planets
Extreme Optics and the Search for Earth-Like Planets

... I am writing to inform you of exciting new developments for TPF. As part of the Presidents new vision for NASA, the agency has been directed by the President to conduct advanced telescope searches for Earth-like planets and habitable environments around other stars. Dan Coulter, Mike Devirian, and I ...
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XMM-Newton



The XMM-Newton, also known as the X-ray Multi-Mirror Mission and the High Throughput X-ray Spectroscopy Mission, is an orbiting X-ray observatory launched by ESA in December 1999 on an Ariane 5 rocket. It is named in honor of Sir Isaac Newton. The telescope was placed in a very eccentric 48 hour elliptical orbit at 40°; at its apogee it is nearly 114,000 kilometres (71,000 mi) from Earth, while the perigee is only 7,000 kilometres (4,300 mi).
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