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proposed october viewing list
proposed october viewing list

... CS = Carbon Star, * = Video imaging optional, ** = Video imaging recommended ...
Document
Document

... angular velocity, a tangential vector, ie change in position of star against backdrop (separate from parallax) typically mas/yr • Earth/Sun is a moving frame of reference that needs to be corrected for - heliocentric velocity ...
LIFEPAC® 6th Grade Science Unit 9 Worktext - HomeSchool
LIFEPAC® 6th Grade Science Unit 9 Worktext - HomeSchool

... many things about the stars and the universe that we still are yet to discover; however, by faith, we know that God created all that exists, including the stars and all other objects in the heavens. For Christians, any explanation of the universe and its workings must be compatible with our belief t ...
Milky Way Kinematics, or how we discovered the geometry and
Milky Way Kinematics, or how we discovered the geometry and

... We can measure this rate of shear in disk star motions (how much faster or slower stars orbit with distance toward or away from galactic center). Also need to measure orbital velocity at radius of sun. Li dbl d figured Lindblad fi d out how h to do d this hi last l thing. hi Measure dispersion of s ...
The Search for Another Earth
The Search for Another Earth

... Are there planets similar to the Earth? For centuries, these questions baffled curious minds. Either a positive or negative answer, if found one day, would carry a deep philosophical significance for our very existence in the universe. Although the search for extra-terrestrial intelligence was initiate ...
Star Formation - Leslie Looney
Star Formation - Leslie Looney

... Question The molecules that life uses on Earth are complex. In space a)! no one can hear you scream. b)! complex molecules can not be created. The environment is too harsh. c)! complex molecules, up to 13 atoms, have been detected in large quantities. d)! the only kind of molecules detected are miss ...
Document
Document

... K. They will make use of large, sensitive detector arrays with low-power dissipation array readout electronics. Improvements in sensitivity, stability, array size, and power consumption are sought. In particular, novel doping approaches to extend wavelength response, lower dark current and readout n ...
Planetary exploration
Planetary exploration

... Horizons spacecraft during its July 2015 flyby of Pluto and its three moons. Radio signals will take 4.5 hours to reach Earth. ...
VERA Project : overview and current status
VERA Project : overview and current status

... Simultaneous observations of two adjacent sources can cancel out atmospheric fluctuation target accuracy : 10 micro-arcsec ! Target source ...
Ch. 19 (Starbirth)
Ch. 19 (Starbirth)

... This work is protected by United States copyright laws and is provided solely for the use of instructors in teaching their courses and assessing student learning. Dissemination or sale of any part of this work (including on the World Wide Web) will destroy the integrity of the work and is not permit ...
J.Marque: Mode matching of the Virgo FP cavities
J.Marque: Mode matching of the Virgo FP cavities

... o Hope to get good results soon! Goal is a coupling better than 99% for FP cavities. o Mode matching of the IMC to be done soon (coupling is currently 82%). Simulation already done with Finesse. Results show that astigmatism is not critical for such a short cavity. Goal is 98%. ...
Our Galaxy, the Milky Way Galaxy
Our Galaxy, the Milky Way Galaxy

... Gas permeates the entire Milky Way Galaxy (and any other galaxy) o 75% atomic hydrogen (just hydrogen atoms) and 25% helium o Known as ISM (aka Interstellar Medium) o Gas does not even feel gravity (because it is so diffuse) o Gas is moving around randomly because of this o Radiation pressure is pus ...
What theories account for the origin of the solar system?
What theories account for the origin of the solar system?

... Computer simulations show that Jovian planets can grow by direct gas accretion without forming rocky ...
nasafinal - University of Oregon
nasafinal - University of Oregon

Autostar Manual
Autostar Manual

... fastest. Speed settings remain until changed by pressing a different number. Take time now to move the telescope using the ARROW keys. Pick an object and point the telescope at it. Use a slower speed when nearing the object to accurately center it in the viewfinder and then in the eyepiece. These sk ...
The Official Magazine of the University Of St Andrews Astronomical Society 1
The Official Magazine of the University Of St Andrews Astronomical Society 1

Ch 28 Class Notes
Ch 28 Class Notes

... _____________ ______________________________________________________________________________, by knowing the angle between two observed positions and the distance between the observation points. To express these measurements, astronomers use a special unit of distance called a ______________. A pars ...
Mauna Kea Curriculum - Center on Disability Studies
Mauna Kea Curriculum - Center on Disability Studies

... Meteoroid: Large rock (but much smaller than minor planets) moving in an orbit in the solar system. Meteoroids that enter in the Earth’s atmosphere are termed meteors or meteorites, depending on their behavior. Milky Way: Bright band that stretches across the sky, produced by large number of stars a ...
Stars 3
Stars 3

... concentrated toward the edges of the nebula are remnants of the star that were ejected into space by the explosion. At the center of the Crab Nebula lies the Crab Pulsar -- the collapsed core of the exploded star. The Crab Pulsar is a rapidly rotating neutron star – an object only about six miles ac ...
Gov Aker Telescope Operators Manual
Gov Aker Telescope Operators Manual

... The Gov Aker telescope was manufactured by the Tinsley Telescope corporation, and is often referred to as the “Tinsley Telescope”. It is a research class telescope that was previously used on Kitt Peak, and was donated by Steward Observatory, University of Arizona, for public education at Discovery ...
Astronomical Filters on Skynet Telescopes
Astronomical Filters on Skynet Telescopes

... researchers because the numbers can be calibrated. For this reason, we recommend that you use these filters by default. With more filters, more things can be measured Many other things can be done with measurements of colors. For example, if a star is behind a cloud of interstellar dust, it will loo ...
Studying the Universe Studying the Universe
Studying the Universe Studying the Universe

... are called reflecting telescopes. Light enters the telescope and is reflected from a large, curved mirror to a focal point above the mirror. A focal point is the point on the axis of a mirror or lens through which parallel light rays are focused. As shown in Figure 8, reflecting telescopes use a sec ...
Optical instability of the earth`s atmosphere
Optical instability of the earth`s atmosphere

... hemisphere. Such peculiarities are largely due to geophysical properties of the Earth; namely, the sphericity and the axial inclination to the plane of the ecliptic. To examine astroclimate conditions of the world's largest observatories in more detail, we constructed a comparison table (Table 1) l ...
Planetary Systems as Potential Sites for Life
Planetary Systems as Potential Sites for Life

Interdisciplinary Evolution of the Hubble Space Telescope
Interdisciplinary Evolution of the Hubble Space Telescope

... transformational projects quickly and “Big Science” is born. Some scientists learn how to play the game and extend themselves to be activists for important programs. One of these, an astronomer, is Lyman Spitzer, Jr. ...
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Spitzer Space Telescope



The Spitzer Space Telescope (SST), formerly the Space Infrared Telescope Facility (SIRTF), is an infrared space observatory launched in 2003. It is the fourth and final of the NASA Great Observatories program.The planned mission period was to be 2.5 years with a pre-launch expectation that the mission could extend to five or slightly more years until the onboard liquid helium supply was exhausted. This occurred on 15 May 2009. Without liquid helium to cool the telescope to the very low temperatures needed to operate, most of the instruments are no longer usable. However, the two shortest-wavelength modules of the IRAC camera are still operable with the same sensitivity as before the cryogen was exhausted, and will continue to be used in the Spitzer Warm Mission. All Spitzer data, from both the primary and warm phases, are archived at the Infrared Science Archive (IRSA).In keeping with NASA tradition, the telescope was renamed after its successful demonstration of operation, on 18 December 2003. Unlike most telescopes that are named after famous deceased astronomers by a board of scientists, the new name for SIRTF was obtained from a contest open to the general public.The contest led to the telescope being named in honor of astronomer Lyman Spitzer, who had promoted the concept of space telescopes in the 1940s. Spitzer wrote a 1946 report for RAND Corporation describing the advantages of an extraterrestrial observatory and how it could be realized with available or upcoming technology. He has been cited for his pioneering contributions to rocketry and astronomy, as well as ""his vision and leadership in articulating the advantages and benefits to be realized from the Space Telescope Program.""The US$800 million Spitzer was launched from Cape Canaveral Air Force Station, on a Delta II 7920H ELV rocket, Monday, 25 August 2003 at 13:35:39 UTC-5 (EDT).It follows a heliocentric instead of geocentric orbit, trailing and drifting away from Earth's orbit at approximately 0.1 astronomical unit per year (a so-called ""earth-trailing"" orbit). The primary mirror is 85 centimeters (33 in) in diameter, f/12, made of beryllium and is cooled to 5.5 K (−449.77 °F). The satellite contains three instruments that allow it to perform astronomical imaging and photometry from 3 to 180 micrometers, spectroscopy from 5 to 40 micrometers, and spectrophotometry from 5 to 100 micrometers.
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