
The Expanding Universe
... The universe started with a sudden appearance of energy which consequently became matter and is now everything around us. There were two theories regarding the universe The Steady State Universe: where the universe had always been and would always continue to be in ...
... The universe started with a sudden appearance of energy which consequently became matter and is now everything around us. There were two theories regarding the universe The Steady State Universe: where the universe had always been and would always continue to be in ...
Exam 3 Study Guide
... This guide is meant to assist with studying for Exam 3 on March 27, 2017. However, it is not comprehensive. This guide includes topic which might not be on this exam (but which might be on the final). It is also possible that something not specifically mentioned on the guide may be on the exam. Howe ...
... This guide is meant to assist with studying for Exam 3 on March 27, 2017. However, it is not comprehensive. This guide includes topic which might not be on this exam (but which might be on the final). It is also possible that something not specifically mentioned on the guide may be on the exam. Howe ...
Lecture 1 - Department of Physics and Astronomy
... over time or from place to place. Thought Experiment: imagine two teams of scientist measuring the speed of a beam of light. One team measures the speed from a ground. The second team measures the speed from a fast moving airplane following the light beam. Do the two ...
... over time or from place to place. Thought Experiment: imagine two teams of scientist measuring the speed of a beam of light. One team measures the speed from a ground. The second team measures the speed from a fast moving airplane following the light beam. Do the two ...
Chapter 26
... Section 1: Observing the Universe Section 2: Evolution of Stars Section 3: Galaxies and the Milky Way ...
... Section 1: Observing the Universe Section 2: Evolution of Stars Section 3: Galaxies and the Milky Way ...
Lecture 1 Coordinate Systems - Department of Physics & Astronomy
... Sidereal Period (P) Time interval to complete one orbit relative to the background stars ...
... Sidereal Period (P) Time interval to complete one orbit relative to the background stars ...
Where do we come from?
... We see galaxies with large redshift (implying large distance, implying distant past). ...
... We see galaxies with large redshift (implying large distance, implying distant past). ...
new_qwk11
... ruler is measured to be longer than its twin ruler at rest D. The mass or inertia of an object decreases when its speed approaches the speed of light ...
... ruler is measured to be longer than its twin ruler at rest D. The mass or inertia of an object decreases when its speed approaches the speed of light ...
SPACE EXPLORATION UNIT
... Using computers to combine images from >1 telescope Acts like telescope the size of the distance between telescopes (greatly improves resolving power) The Very Large Telescope (VLT) is operated by the European Southern Observatory in Chile ...
... Using computers to combine images from >1 telescope Acts like telescope the size of the distance between telescopes (greatly improves resolving power) The Very Large Telescope (VLT) is operated by the European Southern Observatory in Chile ...
Contributions of astronomy to all of science
... you will have the scale on which galaxies group together in clusters of clusters. These are the largest structures of the Universe, which are scattered like so many continents across the emptiness of the cosmos. ...
... you will have the scale on which galaxies group together in clusters of clusters. These are the largest structures of the Universe, which are scattered like so many continents across the emptiness of the cosmos. ...
galaxies
... • has about 200 billion stars, and lots of gas and dust • is a barred-spiral (we think) • about 100,000 light-years wide • our Sun is halfway to the edge, revolving at half a million miles per hour around the center of the Galaxy • takes our Solar System about 200 million years to revolve once aroun ...
... • has about 200 billion stars, and lots of gas and dust • is a barred-spiral (we think) • about 100,000 light-years wide • our Sun is halfway to the edge, revolving at half a million miles per hour around the center of the Galaxy • takes our Solar System about 200 million years to revolve once aroun ...
The Hubble Ultra Deep Field Project Overview
... The velocity you calculated for this star is much less than the speed of light, so we could have found a decent approximation to the answer using z = v/c. But, if you use the approximation equation to calculate the recession velocity based on the spectral shift from the spectrum of a distant galaxy ...
... The velocity you calculated for this star is much less than the speed of light, so we could have found a decent approximation to the answer using z = v/c. But, if you use the approximation equation to calculate the recession velocity based on the spectral shift from the spectrum of a distant galaxy ...
File
... determines how fast the cloud will form a disk before it is completely turned into stars Protogalactic cooling…the initial density determines how fast the cloud can form stars before it collapses ...
... determines how fast the cloud will form a disk before it is completely turned into stars Protogalactic cooling…the initial density determines how fast the cloud can form stars before it collapses ...
Handout from Allaire Star Party
... Earth would be about the size of a pea. If you placed the beach ball on one goal line of a football field, the Earth would be at about the fifty-yard line. Pluto would be about 20 football fields away from the Sun. How far away are the closest stars? Imagine now that the Sun is shrunk even further, ...
... Earth would be about the size of a pea. If you placed the beach ball on one goal line of a football field, the Earth would be at about the fifty-yard line. Pluto would be about 20 football fields away from the Sun. How far away are the closest stars? Imagine now that the Sun is shrunk even further, ...
Astronomy and Our Origins
... Where did we come from? • Scientists believe the entire universe began as a single, one dimensional speck that exploded into existence. • This idea is called the Big Bang Theory! • Do we know for sure…of course not…we could be right or wrong. We will never know. • But we do have a lot of evidence t ...
... Where did we come from? • Scientists believe the entire universe began as a single, one dimensional speck that exploded into existence. • This idea is called the Big Bang Theory! • Do we know for sure…of course not…we could be right or wrong. We will never know. • But we do have a lot of evidence t ...
Galaxies and the Universe bb
... • Outermost stars move the slowest • Sun rotates around the galactic nucleus once about every 200 million years ...
... • Outermost stars move the slowest • Sun rotates around the galactic nucleus once about every 200 million years ...
Lecture 7 Stars and Galaxies and Nebula, (Oh My!) Feb 18 2003
... They orbit in the disk of our galaxy and don't last very long, members escape the group over time. All about the same age and composition so it is likely that they formed around the same time. ...
... They orbit in the disk of our galaxy and don't last very long, members escape the group over time. All about the same age and composition so it is likely that they formed around the same time. ...
Not a limitation
... • EVERYTHING was in one small point (singularity) that “blew up” and is still moving outwards today • Not really an explosion, so much as a very rapid expansion…like blowing up a balloon • About 13.7 billion years ago • Microwave radiation detected in the 1960’s supports this theory. It’s left over ...
... • EVERYTHING was in one small point (singularity) that “blew up” and is still moving outwards today • Not really an explosion, so much as a very rapid expansion…like blowing up a balloon • About 13.7 billion years ago • Microwave radiation detected in the 1960’s supports this theory. It’s left over ...
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.