
5-E Galaxy T - McDonald Observatory
... Do you think galaxies collide? Why or why not? Galaxies, compared to their size, are closer together than stars. They are also much more massive, having the combined mass of billions of stars. So, even over a large distance the force of gravity between galaxies can accelerate them toward each other. ...
... Do you think galaxies collide? Why or why not? Galaxies, compared to their size, are closer together than stars. They are also much more massive, having the combined mass of billions of stars. So, even over a large distance the force of gravity between galaxies can accelerate them toward each other. ...
Tools of Astronomy
... 3. Proxima Centauri is our nearest star. It is ___ light years away! In other words…. It would take light, traveling at a rate that takes it all the way across the United States and halfway back in one second, almost four and a half ________ to get just to the nearest star! 4. Let’s fly out across t ...
... 3. Proxima Centauri is our nearest star. It is ___ light years away! In other words…. It would take light, traveling at a rate that takes it all the way across the United States and halfway back in one second, almost four and a half ________ to get just to the nearest star! 4. Let’s fly out across t ...
Chapter 5 Notes
... A. __________ gravity holds together a large collection of stars, gas, and dust 1. Earth galaxy is Milky Way which is part of a galaxy cluster named the ______ _____. 2. _______ _______ - spiral arms wind out from inner section; some have barred spirals with stars and gas in a central bar 3. _______ ...
... A. __________ gravity holds together a large collection of stars, gas, and dust 1. Earth galaxy is Milky Way which is part of a galaxy cluster named the ______ _____. 2. _______ _______ - spiral arms wind out from inner section; some have barred spirals with stars and gas in a central bar 3. _______ ...
Searching for the Most Distant Black Holes in the Early
... – each is about half the size of the full moon – 1 million and 2 million seconds with Chandra ...
... – each is about half the size of the full moon – 1 million and 2 million seconds with Chandra ...
Unit Two Worksheet – Astronomy
... It is thought that before the Big Bang, all the matter and energy in the universe was in the form of one ___. (A) extremely small volume (C) solar system (B) expanding cloud (D) galaxy ...
... It is thought that before the Big Bang, all the matter and energy in the universe was in the form of one ___. (A) extremely small volume (C) solar system (B) expanding cloud (D) galaxy ...
Space Explorations - Holy Cross Collegiate
... Radio Telescopes Radio signals come from the sky. Radio astronomers ...
... Radio Telescopes Radio signals come from the sky. Radio astronomers ...
Astronomy and the Universe - Department of Physics and Astronomy
... What makes up our solar system? What are the stars? Do they last forever? What are galaxies? What do astronomers learn by studying them? How does measuring angles help astronomers learn about objects in the sky? What is powers-of-ten notation, and why is it useful in ...
... What makes up our solar system? What are the stars? Do they last forever? What are galaxies? What do astronomers learn by studying them? How does measuring angles help astronomers learn about objects in the sky? What is powers-of-ten notation, and why is it useful in ...
Review Sheet and Study Hints - Tufts Institute of Cosmology
... draw evolutionary tracks in the HRD for stars of different masses comment on relative evolutionary time-scales globular cluster HRD’s main sequence turnoff and ages distance determinations use the HRD to determine star-formation histories in galaxies ...
... draw evolutionary tracks in the HRD for stars of different masses comment on relative evolutionary time-scales globular cluster HRD’s main sequence turnoff and ages distance determinations use the HRD to determine star-formation histories in galaxies ...
Astronomy 10B List of Concepts– by Chapter
... CHAPTER 18 AGN’S, QUASARS • If a QSO is a AGN, what are TLA's? • Quasars are called “quasi Stellar objects” (QSO) • Luminosity, diameter, energy source, distance - age • Seyfert galaxies & Active radio galaxies • Jets CHAPTER 19 GALAXIES, CLUSTERS AND LARGE SCALE STRUCTURE • Definitions (Cosmologica ...
... CHAPTER 18 AGN’S, QUASARS • If a QSO is a AGN, what are TLA's? • Quasars are called “quasi Stellar objects” (QSO) • Luminosity, diameter, energy source, distance - age • Seyfert galaxies & Active radio galaxies • Jets CHAPTER 19 GALAXIES, CLUSTERS AND LARGE SCALE STRUCTURE • Definitions (Cosmologica ...
March 2017 - Shasta Astronomy Club
... Shasta Astronomy Club Newsletter where all the objects were in the fields, separated stars from distant background galaxies (stars are point sources, whereas most galaxies are slightly extended), and then looked for places where there were more stars than expected — hoping some might be faint Milky ...
... Shasta Astronomy Club Newsletter where all the objects were in the fields, separated stars from distant background galaxies (stars are point sources, whereas most galaxies are slightly extended), and then looked for places where there were more stars than expected — hoping some might be faint Milky ...
W > 1 - The Open University
... NGC4374 (M84) (9.3) eg and NGC4406 (M86) (9.2) eg easily visible in the same field of view. Scan this field carefully to locate other non-Messier galaxies. Note their positions and sketch the field, then use a suitable star chart to identify them. NGC4486 (M87) (8.6) eg. About 1o southeast of M84 & ...
... NGC4374 (M84) (9.3) eg and NGC4406 (M86) (9.2) eg easily visible in the same field of view. Scan this field carefully to locate other non-Messier galaxies. Note their positions and sketch the field, then use a suitable star chart to identify them. NGC4486 (M87) (8.6) eg. About 1o southeast of M84 & ...
Winners of the OBAFGKM Mnemonic Quasars & Active Galactic Nuclei—4 April
... something in orbit Speed of ejected material ...
... something in orbit Speed of ejected material ...
Supernova Stalking - Susanna Kumlien Reportage
... a so-called Standard Candle. A Standard Candle is an object astronomers can use to measure distances in the universe, taking advantage of its known properties. With its distance from Earth of only some 12 million light years, considered to be “nearby” by cosmological standards, the supernova´s proxi ...
... a so-called Standard Candle. A Standard Candle is an object astronomers can use to measure distances in the universe, taking advantage of its known properties. With its distance from Earth of only some 12 million light years, considered to be “nearby” by cosmological standards, the supernova´s proxi ...
The Milky Way – A Classic Galaxy
... Discovery of the Milky Way as a Galaxy… • Edwin Hubble used the new 100” Mt. Wilson telescope in the 1920’s to image The Andromeda Nebula • Could see the brightest individual stars. Among them, variables of the right color and light variation to show them as Cepheids • Therefore, this was not a nea ...
... Discovery of the Milky Way as a Galaxy… • Edwin Hubble used the new 100” Mt. Wilson telescope in the 1920’s to image The Andromeda Nebula • Could see the brightest individual stars. Among them, variables of the right color and light variation to show them as Cepheids • Therefore, this was not a nea ...
The Fundamental Plane, Stellar Popula6ons
... Some of the (many) things we don’t know (at least not well)… What is the relaBon between stellar mass and dynamical mass, and how does this vary with parent halo mass & environment? How do the observed trends in stellar populaBons vary with environment (NN/local density/cluster radius/cluster ...
... Some of the (many) things we don’t know (at least not well)… What is the relaBon between stellar mass and dynamical mass, and how does this vary with parent halo mass & environment? How do the observed trends in stellar populaBons vary with environment (NN/local density/cluster radius/cluster ...
30 Doradus - HubbleSOURCE
... The majority of the massive stars are binaries In the crowded core of a star cluster encounters between binaries and a 3rd star are ...
... The majority of the massive stars are binaries In the crowded core of a star cluster encounters between binaries and a 3rd star are ...
Semester #1 – GeoScience Review Guide – Final Exam Scale
... 1. What is a light-year? How big is it in kilometers? 2. In your scale model of the Solar System, the scale was 1 cm = 10,000,000,000 km. Jupiter is 778,000,000 km from the sun. On your scale model, how many cm was Jupiter from the sun? 3. Is this a true or false statement? 104 = 10 x 10 x 10 x 10 4 ...
... 1. What is a light-year? How big is it in kilometers? 2. In your scale model of the Solar System, the scale was 1 cm = 10,000,000,000 km. Jupiter is 778,000,000 km from the sun. On your scale model, how many cm was Jupiter from the sun? 3. Is this a true or false statement? 104 = 10 x 10 x 10 x 10 4 ...
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.