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Full Press Release - The Open University
Full Press Release - The Open University

... stars in the dense gas itself, and emits infrared light. The formation of a new generation of stars is now taking place within this compressed gas in these outer shell structures. The AKARI data reveals for the first time, the detailed distribution of this swept out gas and dust over the entire nebu ...
Our Galaxy -- The Milky Way PowerPoint
Our Galaxy -- The Milky Way PowerPoint

1_Introduction
1_Introduction

Telephone Quizzes for ASTR 200 1999 Revision
Telephone Quizzes for ASTR 200 1999 Revision

... is the same as that of the Sun as mass does not affect the lifetime of a star. is shorter than that of the Sun since there is less fuel to burn. is longer than that of the Sun because the star generates energy (uses fuel) at a very slow rate. cannot be discussed as such a star is too small to genera ...
Great Discoveries in Astronomy and Astrophysics 171.112
Great Discoveries in Astronomy and Astrophysics 171.112

... the mechanics of the course and I welcome suggestions! Some of the course mechanics may be amended during the semester as I seek to improve the experience. ...
Topic 3 Earth in the Universe
Topic 3 Earth in the Universe

- Fermi Gamma-ray Space Telescope
- Fermi Gamma-ray Space Telescope

The Prelude  - Solar Physics and Space Weather
The Prelude - Solar Physics and Space Weather

... electrons and positions annihilated to form low energy gammaray photons that can not reverse the process •As a result, matter and anti-matter content decreased, and radiation content increased •From 1 second to 380,000 years, the universe is dominated by the radiation (so called primordial fireball) ...
Wandering in the Redshift Desert
Wandering in the Redshift Desert

The resolved stellar populations of M32 Monachesi, Antonela
The resolved stellar populations of M32 Monachesi, Antonela

... The analysis presented in Chapter 2 helped to constrain the ages and metallicities of M32 at our field location. However, a quantitative determination of the mix of ages and metallicities, which would provide more detailed information about its SFH, requires a deeper analysis. This is done in Chapte ...
Galaxies (and stars) in the far infrared: results from the AKARI All
Galaxies (and stars) in the far infrared: results from the AKARI All

... wavelengths), and this cannot be a trivial application of IRAS methodology, since the physical processes behind emission in these bands are different. ...
Summary: Nuclear burning in stars
Summary: Nuclear burning in stars

... • Spiral arms have higher density than space between arms • Excess gravitational attraction slows down gas, stars when they pass through spiral arm in course of their orbits. • Î spiral arms are a traffic jam ...
Astronomy Jeopardy Astronomy jeopardy
Astronomy Jeopardy Astronomy jeopardy

... When there is equilibrium between the stellar fusion pushing out and the gravity pulling in the star is called… (Hint: our sun is this type of star) ...
Earth`s Motions
Earth`s Motions

... object • happens because of tidal forces that cause the precession of the equinoxes to vary over time so that the speed of precession is not constant • principal sources of tidal force are the Sun and Moon, which continuously change location relative to each other and thus cause nutation in Earth's ...
Volume 20 Number 5 April 2012 - Forsyth Astronomical Society
Volume 20 Number 5 April 2012 - Forsyth Astronomical Society

... the most distant cluster of red galaxies ever observed. It is located 10.5 billion light years away in the direction of the constellation LEO. The cluster is made up of 30 galaxies packed closely together, forming the earliest known "galaxy city" in the universe. They used a new technique which allo ...
Grade 6 Standard 4 - Murray School District
Grade 6 Standard 4 - Murray School District

... Standard 4: Students will understand the scale of size, distance between objects, movement, and apparent motion (due to Earth’s rotation) of objects in the universe and how cultures have understood, related to and used these objects in the night sky. Objective 2: Describe the appearance and apparent ...
Barred Spiral Galaxy
Barred Spiral Galaxy

... • Large amounts of electrically charged gas are ejected suddenly from the Sun’s corona. ...
56.Kirkpatrick_sci_hi
56.Kirkpatrick_sci_hi

... Why are subdwarf brown dwarfs important? Star Formation: These discoveries show further evidence that lowmetallicity clouds still produce very low-mass objects. Although more of these very cool subdwarfs are needed before that formation efficiency can be compared to brown dwarf formation at current ...
Option: Astrophysics Objects in the Universe: Asteroid: a small rocky
Option: Astrophysics Objects in the Universe: Asteroid: a small rocky

AAS Poster, NM 2002: "The Discovery of New
AAS Poster, NM 2002: "The Discovery of New

... Figure 2. Potential WR candidates: Asterisks indicate new detections, squares are spectroscopically confirmed WR stars and diamonds are the “control field”. The smallest ellipse contains likely non-WR stars. Progressing in size, the next region contains 25 questionable candidates, followed by a larg ...
Review Guide
Review Guide

... 15. What force causes stars to form? 16. What do we call a beginning star that is not yet hot enough to engage in nuclear fusion? 17. What is the main fuel source of stars? Which element? ...
ULTRASAT in a nutshell (Feb 2017)
ULTRASAT in a nutshell (Feb 2017)

Powerpoint
Powerpoint

Our Place in the Universe (Chapter 1) The Structure and Size of the
Our Place in the Universe (Chapter 1) The Structure and Size of the

... • How are Earth, the solar system, and galaxies moving? – Earth rotates on its axis once per day and orbits the Sun once each year. Earth’s axis is tilted from its orbital plane – Everything in the solar system orbits the Sun. The Sun orbits the centre of the Milky Way – Galaxies are receding from e ...
Ch17_Galaxies
Ch17_Galaxies

... – Census of galaxies nearby: Most are dim dwarf E and dwarf Irr sparsely populated with stars – Census of distant galaxies: In clusters, 60% of members are spirals and S0, while in sparsely populated regions it is 80% – Early (very young) galaxies are much smaller than Milky Way – merging of these s ...
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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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