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docx - STAO
docx - STAO

... Students could use their astrolabes to collect data observing the change in position of the Moon, Polaris, and other celestial objects in the night sky. Depending on the season you could direct students to observe specific celestial objects, e.g., Jupiter, Betelgeuse, other stars of Orion in the win ...
information on Astronomy Basics and
information on Astronomy Basics and

... (or R.A. for short). Like the Earth’s lines of longitude, they run from pole to pole and are evenly spaced 15 degrees apart. Although the longitude lines are separated by an angular distance, they are also a measure of time. Each line of longitude is one hour apart from the next. Since the Earth rot ...
Calculating Parallax Lab
Calculating Parallax Lab

... 12. Parallax is only one method (known as “standard candles”) to determine the distance to nearby stars. There are several other methods that are used by astronomers. These methods each have their own specific technique and purpose, with some overlap to help confirm accuracy of other methods. Look a ...
30-1 - Fremont Peak Observatory Association
30-1 - Fremont Peak Observatory Association

... Right before the bright part of the Milky Way makes its appearance there are several bright globs in Ophiuchus. Technically this is the bulge of the Milky Way, but seeing the bulge requires an exceptionally dark sky. M 10, 12, and 14 are all an easy star hop from each other. There are also several b ...
Is the central binary system of the planetary nebula Henize 2
Is the central binary system of the planetary nebula Henize 2

... in Abell 48 whose central star is a WN star (Todt et al., 2013). Most interestingly, in the study by Weidmann and Gamen (2011) there are several PNe that show a wide He II 5412 Å absorption line with a weak emission feature in the center of the wide absorption line. This forms a spectral structure ...
The Science of Astronomy
The Science of Astronomy

... Venus, Mars, Jupiter, Saturn. Note that the ancient definition of planet (which meant “wandering star”) applied to any object that appeared to wander among the fixed stars. That is why the Sun and Moon were on the list while Earth was not, because we don’t see our own planet moving in the sky. think ...
UniverseofGalaxies
UniverseofGalaxies

... discovers the periodluminosity relation for Cepheid variable stars. ...
Your Star:  _____________________ Write down the wavelength at which the one
Your Star: _____________________ Write down the wavelength at which the one

... Autumn Stars – The stars of fall are not very well-known. Capella is a double system containing two nearly-identical stars with temperatures very similar to the Sun's; Epsilon Eridani is a faint star with the distinction of having a recently discovered planet orbiting it. Name ...
Infrared spatial interferometer (ISI) scientists, technicians, students
Infrared spatial interferometer (ISI) scientists, technicians, students

... Geometric delays removed using RF delay lines. Currently located at Mt. Wilson Observatory, a site noted for very stable seeing. Two telescopes in operation 1988 First fringes 1989 Third telescope 2003 Closure phase measured 2004 ...
Comets, vagrants of the universe
Comets, vagrants of the universe

... Comets travel in elliptical orbits elongated and in a different plane of the Solar System. They move at high speed, increasing as they approach the Sun, because the gravity that attracts them is greater; they move more slowly in its remote orbit. Comets can be classified by time in describing its or ...
10 Astrophysics (Option E)
10 Astrophysics (Option E)

... planets and their moons, asteroids and comets. When modelling gravity, we treated orbits as circular for simplicity, but in fact, the planets have slightly elliptical orbits. An ellipse is a flattened circle with two centres; one of these centres is the Sun. We know that for a satellite to have a ci ...
File
File

... Not all electromagnetic radiation coming from space reaches the Earth's surface. The diagram shows how far radiation from each part of the electromagnetic spectrum travels down through the atmosphere. ...
The Origin, Structure, and Evolution of the Stars
The Origin, Structure, and Evolution of the Stars

Galileo galilei
Galileo galilei

... Galileo Galilei is an Italian astrometry. He started being an astrometry in the year of 1504. Did you know how he did it? It started when he heard about the new invention from Holland, telescope. He was interested with the telescope, so he decided to make his own telescope. When Galileo Galilei star ...
12 The Milky Way - Journigan-wiki
12 The Milky Way - Journigan-wiki

... correctly placed the Sun within the galaxy, but he grossly overestimated the size. Kapteyn came closer to the actual size of our Galaxy. Neither knew of the attenuating effects of interstellar gases. Neither knew that there were two types of variable stars. Looking back at the controversy, it’s funn ...
The Galactic evolution of phosphorus
The Galactic evolution of phosphorus

... therein). This is not the case for phosphorus, that, before this work, had never been analysed systematically in cool stars. The reason why was already given by Struve (1930): no P i line is available in the “ordinary” range of the observed spectra of stars of spectral type F, G, or K. Some P ii and ...
Properties of Ellipticals and Spirals
Properties of Ellipticals and Spirals

... Blue stars are still on main sequence The most luminous stars, i.e., the blue, hot, and young stars have evolved off the main sequence and have terminated their lives. ...
Project 8 : Stellar Spectra: Classification
Project 8 : Stellar Spectra: Classification

... Absorption  lines  occur  when  an  electron  absorbs  energy  from  the  spectrum  to  move  up  the  energy  levels  in  the  atom.  Since  hydrogen  has  only  one  electron,  this  electron  is  usually  in  the  ground  state.  But  as  the  temperature  rises,  the  average  electron  gains  m ...
The Copernican revolution - University of Florida Astronomy
The Copernican revolution - University of Florida Astronomy

- Astronomical Society of the Pacific
- Astronomical Society of the Pacific

... and the Asteroid Belt, and it has an encounter with Jupiter coming up on February 28, 2007. Not bad for it’s first year of flight, right? But the long haul to Pluto will take another 8 years — yes, the Solar System is really, really big. The New Horizons science team wants to reach the Pluto system as ...
Summary Of the Structure of the Milky Way
Summary Of the Structure of the Milky Way

... used as standard candles to measure galactic distances. • This type of variable is named after the prototype, the variable star RR Lyrae in the constellation Lyra. • RR Lyraes are pulsating horizontal branch stars of spectral class A (and sometimes F), with a mass of around half the Sun's. • RR Lyra ...
previous lectures - Gwynedd Astronomy Society
previous lectures - Gwynedd Astronomy Society

... J Mithan The Astronomical slate carvings of Dyffryn Ogwen ...
Harappan Astronomy
Harappan Astronomy

... went through a complex evolutionary pattern (Vahia and Yadav, 2011a). It was the most advanced preiron civilisation in the world. It is no surprise, therefore, that the Harappans had a vibrant intellectual tradition. This can be seen in their art work (Vahia and Yadav, 2011b) and writing (see e.g. Y ...
Hubble`s Constant - Scientific Research Publishing
Hubble`s Constant - Scientific Research Publishing

... The most obvious feature of the Big Bang cosmological model [3] [4] is its statement that the Cosmos began at some definite past time; in such a way that the expansion rate determines the age of the Universe. Hubble’s constant measures how fast is the process of the expansion, and it is involved in ...
THE DAWN OF X-RAY ASTRONOMY
THE DAWN OF X-RAY ASTRONOMY

... in 1972 that black holes would have masses greater than 3.4 times the mass of the Sun (Rhoades and Ruffini, 1974).27 Thus we could reach conclusions regarding Cyg X–1: the Cyg X–1 x–ray emitter is a compact object of less than 30 km radius due to the rapidity of the pulsations and the fact that the ...
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International Ultraviolet Explorer



The International Ultraviolet Explorer (IUE) was an astronomical observatory satellite primarily designed to take ultraviolet spectra. The satellite was a collaborative project between NASA, the UK Science Research Council and the European Space Agency (ESA). The mission was first proposed in early 1964, by a group of scientists in the United Kingdom, and was launched on January 26, 1978 aboard a NASA Delta rocket. The mission lifetime was initially set for 3 years, but in the end it lasted almost 18 years, with the satellite being shut down in 1996. The switch-off occurred for financial reasons, while the telescope was still functioning at near original efficiency.It was the first space observatory to be operated in real time by astronomers who visited the groundstations in the United States and Europe. Astronomers made over 104,000 observations using the IUE, of objects ranging from solar system bodies to distant quasars. Among the significant scientific results from IUE data were the first large scale studies of stellar winds, accurate measurements of the way interstellar dust absorbs light, and measurements of the supernova SN1987A which showed that it defied stellar evolution theories as they then stood. When the mission ended, it was considered the most successful astronomical satellite ever.
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