
AST 207 Test 3 23 November 2009
... a. (1 pt.) At the present time, does the value of Hubble’s constant depend on the galaxy in which the observations are made? (2 pts.) Explain your reasoning. b. Simplicio erroneously believes that everything in the universe is expanding according to Hubble’s Law. At an earlier time, everything did o ...
... a. (1 pt.) At the present time, does the value of Hubble’s constant depend on the galaxy in which the observations are made? (2 pts.) Explain your reasoning. b. Simplicio erroneously believes that everything in the universe is expanding according to Hubble’s Law. At an earlier time, everything did o ...
Small Wonders: Andromeda
... globulars in our own galaxy at this point - now it's time to take a peek at the brightest globular in the local group. The catch? It's not in our galaxy. It's in Andromeda. The shot to the left was taken by the Hubble Space Telescope. It's called G1 or Mayall II and orbits the Andromeda Galaxy at a ...
... globulars in our own galaxy at this point - now it's time to take a peek at the brightest globular in the local group. The catch? It's not in our galaxy. It's in Andromeda. The shot to the left was taken by the Hubble Space Telescope. It's called G1 or Mayall II and orbits the Andromeda Galaxy at a ...
1 UNIT 3 EARTH HISTORY - POSSIBLE TEST QUESTIONS OUR
... 14. How fast does light travel in miles per second? 15. What can travel faster than light? Galaxies 16. Who first proved that galaxies are located outside our own galaxy? 17. Give a simple definition of a galaxy Galaxy Types 18. What three galactic types make up the Hubble classification of galaxies ...
... 14. How fast does light travel in miles per second? 15. What can travel faster than light? Galaxies 16. Who first proved that galaxies are located outside our own galaxy? 17. Give a simple definition of a galaxy Galaxy Types 18. What three galactic types make up the Hubble classification of galaxies ...
Stars and Galaxies
... Now show me 50 centimeters. Now tell me (without thinking about it, or calculating it in meters) how far 500 centemeters is. 2000? 20,000? We need numbers that make sense to us in relationship to objects; we scale up and use meters and kilometers for large numbers. ...
... Now show me 50 centimeters. Now tell me (without thinking about it, or calculating it in meters) how far 500 centemeters is. 2000? 20,000? We need numbers that make sense to us in relationship to objects; we scale up and use meters and kilometers for large numbers. ...
E N 1”=140 AU
... north (P.A. ~20 deg) of the binary system. Its structure is the following: ・The bubble extending with time ・[S II], Hα, and [O I] emission lines ・The bubble = Shock created by collision between circumstellar material and jet from the primary?? ・Accretion from the circumstellar disk around the primar ...
... north (P.A. ~20 deg) of the binary system. Its structure is the following: ・The bubble extending with time ・[S II], Hα, and [O I] emission lines ・The bubble = Shock created by collision between circumstellar material and jet from the primary?? ・Accretion from the circumstellar disk around the primar ...
Pointing Model for the Large Millimeter Telescope Computational Physics Project 2
... To fit this linear model, we use the standard least squares approach described in class. ...
... To fit this linear model, we use the standard least squares approach described in class. ...
Chapter 25 PowerPoint
... The light hitting the earth right now is 30 thousand years old. The energy in the sunlight we see today started out in the core of the Sun 30,000 years ago – it spent most of this time passing through the dense atoms that make the sun and just 8 minutes to reach us once it had left the Sun! The temp ...
... The light hitting the earth right now is 30 thousand years old. The energy in the sunlight we see today started out in the core of the Sun 30,000 years ago – it spent most of this time passing through the dense atoms that make the sun and just 8 minutes to reach us once it had left the Sun! The temp ...
2011 - Edexcel
... Some questions must be answered with a cross in the box ( ). If you change your mind about an answer, put a line through the box ( ) and then mark your new answer with a cross ( ). 1 (a) Which of these objects in the Solar System has the smallest diameter? ...
... Some questions must be answered with a cross in the box ( ). If you change your mind about an answer, put a line through the box ( ) and then mark your new answer with a cross ( ). 1 (a) Which of these objects in the Solar System has the smallest diameter? ...
PowerPoint Presentation - Center for Gravitational Wave Physics
... and the star formation rate, allowing for 1. Improved understanding of the Fe abundance in galaxy clusters, 2. Ia rate as a function of redshift, 3. Clear evidence for multiple progenitors ...
... and the star formation rate, allowing for 1. Improved understanding of the Fe abundance in galaxy clusters, 2. Ia rate as a function of redshift, 3. Clear evidence for multiple progenitors ...
fred`s 2017 astronomy challenge
... in December, there are hundreds upon thousands of interesting things in the night-‐time sky. I have listed top twenty things that I challenge the members of the society to view. For the more experie ...
... in December, there are hundreds upon thousands of interesting things in the night-‐time sky. I have listed top twenty things that I challenge the members of the society to view. For the more experie ...
OCR Physics A Refer to the Physics A datasheet for data, formulae
... © Oxford University Press 2016 http://www.oxfordsecondary.co.uk/acknowledgements This resource sheet may have been changed from the original ...
... © Oxford University Press 2016 http://www.oxfordsecondary.co.uk/acknowledgements This resource sheet may have been changed from the original ...
Project Descriptions - UCI Physics and Astronomy
... known as “blinking” in order to identify asteroids in the field. Even though asteroids are much smaller than stars, they are also much closer, which makes them appear as infinitely small, star-like objects when imaged with a telescope. This makes their identification confusing, as they can often be ...
... known as “blinking” in order to identify asteroids in the field. Even though asteroids are much smaller than stars, they are also much closer, which makes them appear as infinitely small, star-like objects when imaged with a telescope. This makes their identification confusing, as they can often be ...
the summary
... A GRB afterglow can be observed over a broad range of wavelengths: from X-rays, ultraviolet to optical, infrared and radio waves. All of this radiation is light; only the energy per photon (or equivalently wavelength, or frequency) is different. While the initial gamma-rays are observed from space w ...
... A GRB afterglow can be observed over a broad range of wavelengths: from X-rays, ultraviolet to optical, infrared and radio waves. All of this radiation is light; only the energy per photon (or equivalently wavelength, or frequency) is different. While the initial gamma-rays are observed from space w ...
M81/M82/NGC3077
... (CBR value: 48 km/sec) M82 — 202 km/sec (3.9 ± 0.3 Mpc) (CBR value: 296 km/sec) M81 is closer and approaching, while M82 is farther away and receding; ...
... (CBR value: 48 km/sec) M82 — 202 km/sec (3.9 ± 0.3 Mpc) (CBR value: 296 km/sec) M81 is closer and approaching, while M82 is farther away and receding; ...
Extragalactic Distances from Planetary Nebulae
... [Ciardullo et al.] • 1990: First PNLF-based Hubble Constant [Jacoby et al.] • 1990: First Use of the PNLF in the Galaxy [Pottasch] ...
... [Ciardullo et al.] • 1990: First PNLF-based Hubble Constant [Jacoby et al.] • 1990: First Use of the PNLF in the Galaxy [Pottasch] ...
Exoplanet, 51 Pegasi b, Solar System, VLT, La Silla. ESOcast
... richest planetary system yet. The system, located over 120 light-years away around the Sun-like star HD 10180, contains at least five exoplanets. There is also tantalising evidence that two more planets may be present in this system, one of which would have the lowest mass ever found. ...
... richest planetary system yet. The system, located over 120 light-years away around the Sun-like star HD 10180, contains at least five exoplanets. There is also tantalising evidence that two more planets may be present in this system, one of which would have the lowest mass ever found. ...
Astro-2: History of the Universe
... Universe The Hubble constant gives us the current expansion rate of the universe, which we can use to estimate the age of the Universe. 1/H0 is approximately equal to 14 Gyr We should test whether this is consistent with the age of “stuff” in the universe. If we found something significantly older t ...
... Universe The Hubble constant gives us the current expansion rate of the universe, which we can use to estimate the age of the Universe. 1/H0 is approximately equal to 14 Gyr We should test whether this is consistent with the age of “stuff” in the universe. If we found something significantly older t ...
Lecture6
... Universe The Hubble constant gives us the current expansion rate of the universe, which we can use to estimate the age of the Universe. 1/H0 is approximately equal to 14 Gyr We should test whether this is consistent with the age of “stuff” in the universe. If we found something significantly older t ...
... Universe The Hubble constant gives us the current expansion rate of the universe, which we can use to estimate the age of the Universe. 1/H0 is approximately equal to 14 Gyr We should test whether this is consistent with the age of “stuff” in the universe. If we found something significantly older t ...
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.