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ASTR101 Unit 10 Assessment Answer Key 1. Mass, luminosity, size
ASTR101 Unit 10 Assessment Answer Key 1. Mass, luminosity, size

... from about 60 solar masses to about 1/12 solar mass, in luminosity from about 1,000,000 to 1/10,000 solar luminosities, in radius from about 1,000 to 1/10 solar radii, in surface temperature from about 35,000 to 3,000 K, and in age, from about 13 billion years to stars that are just now being born. ...
Sample Answer Sheet for The 10 Tourist Wonders of the
Sample Answer Sheet for The 10 Tourist Wonders of the

... As much as 90% of the star’s material can be thrown off during the explosion and, in the process, new (heavier) elements are made, and then distributed at high speed into the Galaxy. In many ways, life on Earth owes its existence to supernovae and the fact that they “recycle” the material of early g ...
GRIS: The GREGOR Infrared Spectrograph
GRIS: The GREGOR Infrared Spectrograph

... GREGOR is a 1.5-meter solar telescope that has been recently installed at the Observatorio del Teide, Tenerife (see Schmidt et al. 2012 for a global summary of the main science objectives and telescope status). With an effective focal length of ∼57.3 m and an image scale of ∼3.6 mm−1 at the scienc ...
the biggest game in the cosmos
the biggest game in the cosmos

... time is the system working while you are trying to do science?”” he asks. ““What fraction of the light your primary mirror collects makes it to your detector? What fraction of the sky can you cover? Right now, these are all small numbers. This is not a mature technology.”” Angel agrees, but remains ...
Distant galaxies and quasars The ages of things Light
Distant galaxies and quasars The ages of things Light

... galaxies it is taking place in ... This, like the quasar evolution, shows a dramatic peak at earlier times ... but somewhat later than the quasars ...
TYPES OF STARS
TYPES OF STARS

... Modified from: http://cas.sdss.org/dr5/en/proj/teachers/basic/spectraltypes/lesson.asp When astronomers look through their telescopes, they see billions of stars. How do they make sense of all these stars? The goal of this problem set is for you to understand that astronomers classify stars on the b ...
Presentation available here - Lunar and Planetary Institute
Presentation available here - Lunar and Planetary Institute

...  All core collapse explosions are asymmetric, maybe produced by magnetic jets. How can this be proved?  Gamma-ray bursts are caused by jets of material moving at nearly the speed of light. Do they mark the birth of black holes?  At least some gamma-ray bursts (and maybe all) arise in supernova ex ...
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EXAM II REVIEW - University of Maryland: Department of

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Universe Discovery Guides: January

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CopernicanRev1
CopernicanRev1

... Explains the precession of Mercury’s perihelion Predicts the existence of Black Holes Supported by many scientists Supported by many testable predictions Can never can be proven but has not been disproven These can always be modified, based on new data/information Exercise: Science or Not Science an ...
Multiple choice test questions 2, Winter Semester
Multiple choice test questions 2, Winter Semester

... 16) What is a standard candle? A) an object for which we are likely to know its true luminosity B) an object for which we can easily measure its apparent brightness C) a class of objects that we know all have exactly the same luminosity D) any star for which we know its exact apparent brightness E) ...
April 2006 Newsletter PDF - Cowichan Valley Starfinders Society
April 2006 Newsletter PDF - Cowichan Valley Starfinders Society

xavier barcons miguel ángel carrera rafael rebolo isaac
xavier barcons miguel ángel carrera rafael rebolo isaac

Astronomy Daystarter Questions
Astronomy Daystarter Questions

... a. December 22 b. June 21 ...
CAAC 2016-09 - Charlotte Astronomer
CAAC 2016-09 - Charlotte Astronomer

... The Formation of the Charlotte Astronomer’s Club and Its’ History: As the club seeks your input for planning purposes, we have a very timely program for our September 16th meeting. When thinking about the future, it is good to remember and reflect on events that led to the formation of the club and ...
Due: January 15, 2014 Name
Due: January 15, 2014 Name

... A type I supernova leaves no remnant star, unlike a type II supernova, which results from the collapse of a massive star's iron core and which leaves a neutron star or a black hole. Furthermore, not all neutron stars are pulsars because the radiation beam of a spinning neutron star might not point t ...
Astronomy Through the Ages: 2 Middle ages through Renaissance
Astronomy Through the Ages: 2 Middle ages through Renaissance

... Copernicus wrote an overview of his model and circulated it among his friends, including high officials of the church in 1514 CE. – It was well received, many including Pope Paul III were eager to learn more about his theory. – But he resisted openly publishing his views over two decades, not wishin ...
The Search for Earth-like Planets: Yes We Can
The Search for Earth-like Planets: Yes We Can

... Premise: If there is intelligent life “out there”, it probably is similar to life as we know it on Earth. ...
Radio Astronomy
Radio Astronomy

... Symbiotic stars (LR/LO < 10-6 for most stars!) “Microquasars”: some X-ray binaries Pulsars Supernova Remnants Radio Galaxies Quasars (and other AGN) ...
Using a distant X-ray source to detect small Transneptunian Objects
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... Use the following data: Diameter of TNO, DTNO = 100 m; Diameter of X-1 pulsar, DX-1 = 20 km. ...
The Galactic Super Star Cluster Westerlund 1
The Galactic Super Star Cluster Westerlund 1

... times the mass of Orion. Therefore, we would have expected diffuse emission with L x = 3x10 35 erg s-1, which is five times more flux than we observe. We suggest that the IMF is nonstandard, as is often claimed for young, massive star clusters. ...
lookbacktime
lookbacktime

... galaxy leave it earlier, later, or at the same time as the nebula in the previous question? Justify your answer. ...
Orbits - Sunny Okanagan
Orbits - Sunny Okanagan

... earth, the sun must move up or down to keep in the same season. • If the sun moves back half an orbit later, earth can flow out of the reverse orbit. • This because earth’s orbit must shift back by the same amount to keep in the same season. • Thus earth’s axis would always point to the pole star, n ...
Chapter5- Light - SFA Physics and Astronomy
Chapter5- Light - SFA Physics and Astronomy

... • In general, larger diameter telescopes have both a greater light-collecting area and a better angular resolution. • Other factors that limit resolution include: – The engineering and construction of the telescope. – Effects of the atmosphere for ground based telescopes. ...
EXPLORATION OF THE KUIPER BELT BY HIGH
EXPLORATION OF THE KUIPER BELT BY HIGH

... them to diffraction profiles of interplanetary objects. The synthetic profiles depend on two parameters: the object’s radius and its distance from the Sun. The synthetic profile is computed assuming a circular orbit and zero-impact parameter. The parameters of the synthetic profiles given in Table 2 ...
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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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