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The Solar System
The Solar System

... • Low mass stars: White Dwarfs • High mass stars: – supernova remnants, expanding at 10,000 km/s – may trigger future star formation? – Neutron stars: mass star but just 10 km across. • Teaspoon weighs 100 million tons! • Seen as Pulsars, flashing beacons in space. ...
User`s Guide to the Sky Notes
User`s Guide to the Sky Notes

... Some things you think are stars are actually distant galaxies that are so far away, the light from its billions of stars has converged to a single point of light. Over time, humans have named stars, measured their relative brightness, and attempted to determine how far away they are, but that is not ...
Apr 2017 - Astronomical Society of Northern New England
Apr 2017 - Astronomical Society of Northern New England

a. What do we mean by a light year?
a. What do we mean by a light year?

Branches of Earth Science
Branches of Earth Science

... Light Year- Astronomers use light years to measure the distances ______________ stars o A light year is the distance that light ______________ in one year  9,460,730,472,580.8 km  5,878,630,000,000 miles Parallax- the apparent change in the ______________ of a star in the sky. o The change is due ...
CHAP
CHAP

... - Cool stars appear _________ in color with a surface temperature of about 3,200 degrees Celsius. - Warm stars appear _____________ in color with a surface temperature of about 5,500 degrees Celsius. - The hottest stars are ____________ in color and have a surface temperature over 20,000 degrees Cel ...
M = 5.5 - The Millstone
M = 5.5 - The Millstone

... stellar distance (by other means). Absolute magnitude, M, expresses the brightness of a star as it would be if it were placed 10 parsecs away. Since all stars would be placed at the same distance, absolute magnitudes show differences in actual luminosities. It is a measure based on stellar analysis ...
What is a Scientist? - Cockeysville Middle School
What is a Scientist? - Cockeysville Middle School

... What pattern exists for main sequence stars based upon these two characteristics? For main sequence stars, as the surface temperature increases, the absolute brightness increases. ESS-5B ...
The Infrared Astronomical Mission AKARI
The Infrared Astronomical Mission AKARI

... (SFU). AKARI is designed as an All-Sky Survey mission in the infrared. The primary purpose of the mission is to provide second-generation infrared catalogues to better spatial resolution and wider spectral coverage than the first catalogues by the Infra-Red Astronomy Satellite (IRAS) mission (Neuge ...
AS2001 - University of St Andrews
AS2001 - University of St Andrews

... Near centre of galaxy: Shorter orbit period--> More passes thru spiral shocks --> More star generations --> m lower --> Z higher. (Also, more infall of IGM on outskirts.) ...
Stellar Brightness Apparent magnitude
Stellar Brightness Apparent magnitude

...  The brightest stars were in group 1 and called them magnitude 1 stars  The stars they could barely see were put into group 6 – magnitude 6 stars  The lower the number, the brighter the star ...
It is only in the past few years that humanity... limits of the heliosphere. A fortunate confluence of missions has... 1. Magnetic Effects in the Heliosheath and Astrosheaths (Prof. Merav...
It is only in the past few years that humanity... limits of the heliosphere. A fortunate confluence of missions has... 1. Magnetic Effects in the Heliosheath and Astrosheaths (Prof. Merav...

... Recent evidence suggests that at a given color or spectral type, magnetically active, low-mass stars may be more luminous than their inactive counterparts. The increase in luminosity could simply be due to spots on the surface making stars appear colder than their fundamental parameters would predic ...
Inquiry Lab: Exploring the Spectrum Intended Learning Outcomes: 1
Inquiry Lab: Exploring the Spectrum Intended Learning Outcomes: 1

... rays). In the case of light, the effect is difficult to demonstrate without using sophisticated instrumentation, because of the very high speed with which light moves. Therefore, while light is the wave of interest to astronomers, this activity will focus primarily on simulations to demonstrate the ...
Stars
Stars

... Life span of a star depends on its size. – Very large, massive stars burn their fuel much faster than smaller stars – Their main sequence may last only a few hundred thousand years – Smaller stars will live on for billions of years because they burn their fuel much more slowly ...
Definition - SchoolNotes
Definition - SchoolNotes

... One of the limits of ground based optical telescopes is the distortion and interference caused by the Earth’s atmosphere. – To alleviate this problem, NASA has designed and launched space based telescopes like the Hubble Space Telescope. ...
70 Thousand Million, Million, Million Stars in Space
70 Thousand Million, Million, Million Stars in Space

... 24 trillion miles (40 trillion km) away. The Sun is a star at the center of our solar system. Its distance from Earth depends on Earth’s position while orbiting the Sun. On average, it is 93 million miles (150 million km) away. Venus’ distance from Earth varies depending on the orbit of both planets ...
The Interstellar Medium
The Interstellar Medium

... • How can you distinguish between a fact and a theory? The matter between the stars is the starting point for the life story of the stars. The next four chapters will trace the birth, life, and death of stars. ...
Terrestrial Planet (and Life) Finder
Terrestrial Planet (and Life) Finder

... Now estimate number of planets with life in our Galaxy (not number with intelligent, communicating life) If we leave out fi and fc (i.e. assume they are unity—all life forms develop our kind of intelligence and technology and try to communicate), we are calculating the number of life-bearing planet ...
Astrophysics
Astrophysics

... A large change in the observer’s position is required to see any appreciable parallax in distant stars. The greatest baseline achievable for a ground-based telescope is the diameter of the Earth’s orbit around the Sun. o The position of a star relative to distant stars is photographed at 6-monthly i ...
the May 2017 Newsletter!
the May 2017 Newsletter!

... started, Io disappeared into occultation i.e it moved into Jupiter’s shadow. Although the disappearance was not observed, it would have occurred before Io reached Jupiter’s limb. Amongst other things, we did a tour of double stars and clusters, and more or less repeated the tour for the later comers ...
Astro history II
Astro history II

... • angles are harder to measure than it looks here! •Concluded earth must orbit much larger sun! ...
stars
stars

... • Stars change over their lifespan just like animals change throughout their life. • Nebula-a large cloud of gas and dust spread out over a large volume of space. • They can have different appearances bright or dark ...
UGS303, Extraterrestrial Life: REVIEW FOR FIRST TEST
UGS303, Extraterrestrial Life: REVIEW FOR FIRST TEST

... stars. What are the advantages and drawbacks of each? Which method works better for planets orbiting close to their star and which works better for planets in large orbits? Describe how searches for transits and microlensing can detect planets. Which method was used to detect most of the new planets ...
etlife_exoplanets - University of Glasgow
etlife_exoplanets - University of Glasgow

... The distance from the Earth to the Sun is 150 million km. It takes sunlight more than eight minutes to travel this distance. ...
Nearest star`s wobbles could reveal Earth`s twin
Nearest star`s wobbles could reveal Earth`s twin

... should be able to pick up the slight stellar wobbles induced by a small, rocky, Earth-like planet. Alpha Centauri lies just over 4 light years away and is the closest star system to the Sun. It appears to be a triple system, with two Sun-like stars orbiting each other relatively closely (about 23 ti ...
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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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