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An introduce of the spectrograph of the GALEX
An introduce of the spectrograph of the GALEX

Document
Document

... is believed to be the remnant of the primordial reball through which the universe made its appearance. In about a million years after the Big Bang, the temperature of this reball decreased from unbelievably high values of more than 1032 K to a few thousand K, and hydrogen and helium gas formed. No ...
file - University of California San Diego
file - University of California San Diego

... a massive object. Such an object acts like a lens--a gravitational lens--distorting passing light rays in such a way that a distant observer may see multiple objects where only one exists. Some astronomers have proposed that strange quasar-like phenomena called BL Lac objects may actually be the res ...
300 MHz - 3 GHz Yes, we`re interested
300 MHz - 3 GHz Yes, we`re interested

SYLLABUS Spring 2012 SCIE 3304, SECTION 001 ASTRONOMY
SYLLABUS Spring 2012 SCIE 3304, SECTION 001 ASTRONOMY

... as a star, measurement of different properties of stars, birth, evolution and death of stars, strange states of matter (neutron stars and black holes), Milky Way Galaxy, study of the Universe beyond our Galaxy, formation and evolution of galaxies. As we consider more distant objects, such as active ...
Extremely Large Telescopes
Extremely Large Telescopes

... FALCON concept (Hammer et al) ...
presentation (PPT format)
presentation (PPT format)

Patterns in the night sky - Laureate International College
Patterns in the night sky - Laureate International College

... A collection of many billions of stars held together by gravity is called a galaxy. There are billions and billions of galaxies in the universe. Our solar system is located in the Milky Way galaxy. ...
The measure of Cosmological distances
The measure of Cosmological distances

PowerPoint
PowerPoint

The Observable Universe: Redshift, Distances and the Hubble-Law
The Observable Universe: Redshift, Distances and the Hubble-Law

... • Hubble-Law can be used to measure distances in the Universe upto z < 0.2. For z > 0,2  quadratatic deviations (see LCDM). • With this method, the Homogeneity and Isotropy of the Universe also follows from the galaxy distribution for Scales s > 200 Mpc. ...
Class 28 (Jun 2) - Physics at Oregon State University
Class 28 (Jun 2) - Physics at Oregon State University

... Missing Mass • We can calculate the mass of the Milky Way by measuring the orbital velocities of dwarf galaxies in orbit around our galaxy. • We can also count the number of stars in the galaxy, and estimate the galactic mass. The two numbers do not agree. By a factor of 10! • Rotation curves do no ...
Multiple Choice, continued
Multiple Choice, continued

... • The galaxy in which we live, the Milky Way, is a spiral galaxy in which the sun is one of hundreds of billions of stars. • Two irregular galaxies, the Large Magellanic Cloud and Small Magellanic Cloud, are our closest neighbors. • These three galaxies are called the Local Group. ...
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SIMULATIONS

... General applicability to systems with arbitrary geometry, in particular those produced in hydrodynmical simulations (evolutionary history, SFRH ..) Subresolution PDF formalism to describe MC/cirrus density field ...
Earth`s Motion and Seasons
Earth`s Motion and Seasons

... The Hubble Telescope is a reflecting telescope with a mirror 2.4 meters in diameter. Because it orbits Earth above the atmosphere, it can produce very detailed images. Hubble images have changed how astronomers view the universe. The most recent addition to NASA’s lineup of telescopes in space is th ...
Chapter 14 - Heritage Christian School
Chapter 14 - Heritage Christian School

... However, the idea that the Earth is the center of the universe runs contrary to ancient religious thought. This is because hell was considered to be at the center of the Earth; therefore, if Earth was the center of the universe, then hell would in fact be at the center of the universe. Secularists l ...
Formation of the Universe Test Review Packet
Formation of the Universe Test Review Packet

... 6.Hubble's Law 7.Big Bang Theory 8.Light Year Concepts: 9.Use the diagram of the electromagnetic spectrum to answer to following questions: a. What wavelength range does human eye see between? b. Which part of the spectrum has longest wavelength? ...
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... USING KEY TERMS The statements below are false. For each statement, replace the underlined term to make a true statement. ...
How Far is far ?
How Far is far ?

... Gravitational lensing is an effect predicted by General Relativity As light travels to Earth from a distant galaxy, it may be bent around an intervening galaxy by the curvature of space, and follow 2 distinct paths to the Earth. By tracking both paths exactly, an estimate can be made of the distanc ...
Study Guide - Universe Exam key 2014-15 v2
Study Guide - Universe Exam key 2014-15 v2

... 1. Describe the model that was used in the activity titled “Our Expanding Universe.” We used a balloon and put dots on it to represent galaxies. a) How was this model useful? Showed us how galaxies move away from each other as it expands. b) Name 2 limitations of this model. It has boundaries and wi ...
Summary of week 1:
Summary of week 1:

Stars and Galaxies
Stars and Galaxies

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Lecture 12: Galaxies View of the Galaxy from within Comparison to

Mon Aug 5, 2013 QUASAR DISCOVERY Quasars were discovered
Mon Aug 5, 2013 QUASAR DISCOVERY Quasars were discovered

... What’s the most distant star you can see? In 1987, there was a supernova in the Large Magellanic Cloud. It appeared as a 2nd magnitude star, (about the brightness of one of the stars of the Big Dipper,) and could be seen easily with the unaided eye. That star was about 160,000 light years away – tha ...
Life Cycle of Stars
Life Cycle of Stars

... bulge is a huge collection of old stars. It is surrounded by spinning disc of newer stars and clumps of gas and dust.  Our solar system is located on the inner edge of one of the spiral arms.  A massive black hole is located at the centre of the Milky Way ...
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Hubble Deep Field



The Hubble Deep Field (HDF) is an image of a small region in the constellation Ursa Major, constructed from a series of observations by the Hubble Space Telescope. It covers an area 2.5 arcminutes across, about one 24-millionth of the whole sky, which is equivalent in angular size to a 65 mm tennis ball at a distance of 100 metres. The image was assembled from 342 separate exposures taken with the Space Telescope's Wide Field and Planetary Camera 2 over ten consecutive days between December 18 and December 28, 1995.The field is so small that only a few foreground stars in the Milky Way lie within it; thus, almost all of the 3,000 objects in the image are galaxies, some of which are among the youngest and most distant known. By revealing such large numbers of very young galaxies, the HDF has become a landmark image in the study of the early universe, with the associated scientific paper having received over 900 citations by the end of 2014.Three years after the HDF observations were taken, a region in the south celestial hemisphere was imaged in a similar way and named the Hubble Deep Field South. The similarities between the two regions strengthened the belief that the universe is uniform over large scales and that the Earth occupies a typical region in the Universe (the cosmological principle). A wider but shallower survey was also made as part of the Great Observatories Origins Deep Survey. In 2004 a deeper image, known as the Hubble Ultra-Deep Field (HUDF), was constructed from a few months of light exposure. The HUDF image was at the time the most sensitive astronomical image ever made at visible wavelengths, and it remained so until the Hubble Extreme Deep Field (XDF) was released in 2012.
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