
Ch 28 Class Notes
... Radio telescopes are often used in arrays (arrangements of multiple telescopes so they can act like one large telescope). In addition to radio waves, astronomers also gather data from ultraviolet light, X rays, gamma rays, and infrared wavelengths when studying celestial objects. Much of these wavel ...
... Radio telescopes are often used in arrays (arrangements of multiple telescopes so they can act like one large telescope). In addition to radio waves, astronomers also gather data from ultraviolet light, X rays, gamma rays, and infrared wavelengths when studying celestial objects. Much of these wavel ...
Astrophotography Manual
... 3. Methods of using the scope effectively 3.1. Alignment of the finder scope Before alignment, the scope should be balanced so that there will be minimal stress on the observer. To alignment it, release all the clamps and slowly let the scope lie on its side. On the other side, adjust the counter we ...
... 3. Methods of using the scope effectively 3.1. Alignment of the finder scope Before alignment, the scope should be balanced so that there will be minimal stress on the observer. To alignment it, release all the clamps and slowly let the scope lie on its side. On the other side, adjust the counter we ...
1” “Sky-Notes” of the Open University Astronomy Club. September
... NGC6888 (11.0) snr. Southwest of M29 this object provides a difficult visual challenge. Dark transparent skies are essential and a nebular filter will help. A good target for CCD imagers. NGC6910 (7.4) oc. Fine open cluster. NGC6913 (M29) (6.6) oc. Large scattered cluster of stars. Surrounding the M ...
... NGC6888 (11.0) snr. Southwest of M29 this object provides a difficult visual challenge. Dark transparent skies are essential and a nebular filter will help. A good target for CCD imagers. NGC6910 (7.4) oc. Fine open cluster. NGC6913 (M29) (6.6) oc. Large scattered cluster of stars. Surrounding the M ...
Galaxy Classification - Starry Night Education
... Milky Way galaxy? a. The plane of the solar system is coincident with the plane of the galaxy. b. The plane of the solar system is perpendicular to that of the Milky Way. c. The plane of the solar system is inclined at a small angle to the plane of the galaxy. d. The angle between the plane of the s ...
... Milky Way galaxy? a. The plane of the solar system is coincident with the plane of the galaxy. b. The plane of the solar system is perpendicular to that of the Milky Way. c. The plane of the solar system is inclined at a small angle to the plane of the galaxy. d. The angle between the plane of the s ...
The thopograpy of Venus revealed at 1 micron
... The purpose of this imaging campaign was to acquire good quality (high resolution and high S/N) images of the Venus nightside, at 1 micron, during some days, to show the nature and properties of the details visible and the amateur equipment potential. Each session started 10 minutes after the sunset ...
... The purpose of this imaging campaign was to acquire good quality (high resolution and high S/N) images of the Venus nightside, at 1 micron, during some days, to show the nature and properties of the details visible and the amateur equipment potential. Each session started 10 minutes after the sunset ...
ASTRONOMY AND ASTROPHYSICS
... nuclear excitation followed by deexcitation, (2) production of neutral pions (and h¡ etc) and their subsequent decay into gamma-rays, (3) bremstrahlung by high energy electrons, (4) inverse-Compton scattering, (5) particle-antiparticle annihilation, and (6) cyclotron line emission in intense magneti ...
... nuclear excitation followed by deexcitation, (2) production of neutral pions (and h¡ etc) and their subsequent decay into gamma-rays, (3) bremstrahlung by high energy electrons, (4) inverse-Compton scattering, (5) particle-antiparticle annihilation, and (6) cyclotron line emission in intense magneti ...
CH. 7 - science1d
... sky might look like what is shown in the image here. All the thousands of twinkling stars we can see from Earth even without a telescope are part of the galaxy we live in, the Milky Way. A galaxy is a collection of hundreds of billions of stars held together by gravity. Therefore, you might be surpr ...
... sky might look like what is shown in the image here. All the thousands of twinkling stars we can see from Earth even without a telescope are part of the galaxy we live in, the Milky Way. A galaxy is a collection of hundreds of billions of stars held together by gravity. Therefore, you might be surpr ...
PH607lec12
... Another unusual structure in the nucleus is catalogued as 359.1-00.5 and appears to be a superbubble with a cluster 200 newborn stars at its heart. Radio wavelengths have revealed a complex structure of ionized gas called the 'mini-spiral'. The mini-spiral is broken down into individual components i ...
... Another unusual structure in the nucleus is catalogued as 359.1-00.5 and appears to be a superbubble with a cluster 200 newborn stars at its heart. Radio wavelengths have revealed a complex structure of ionized gas called the 'mini-spiral'. The mini-spiral is broken down into individual components i ...
Pluto_Friends
... • Hubble mission background • Discovery of Pluto (1930) and moon Charon (1978) • Hubble observations of Pluto: discovery of moons Nix and Hydra (2005) • Planet vote of 2006: planets and “dwarf planets” • History: how many planets are there? • The “problem” of being first: Ceres & Pluto • Hubble obse ...
... • Hubble mission background • Discovery of Pluto (1930) and moon Charon (1978) • Hubble observations of Pluto: discovery of moons Nix and Hydra (2005) • Planet vote of 2006: planets and “dwarf planets” • History: how many planets are there? • The “problem” of being first: Ceres & Pluto • Hubble obse ...
LIGO Star Chart
... reach us, the distance between the two galaxies is getting smaller. Andromeda is moving toward the Milky Way at about 700,000 miles per hour! The best explanation for this is that the Milky Way and Andromeda are in fact a bound pair of galaxies in orbit around one another. Both galaxies are thought ...
... reach us, the distance between the two galaxies is getting smaller. Andromeda is moving toward the Milky Way at about 700,000 miles per hour! The best explanation for this is that the Milky Way and Andromeda are in fact a bound pair of galaxies in orbit around one another. Both galaxies are thought ...
Chapter 1 - Princeton University Press
... Hubble studied the Andromeda Nebula, which had been thought by many, including Shapley, to be a gas cloud within the Milky Way. The word nebula comes from the Latin nubes, or “cloud,” denoting the fuzzy appearance of these objects. By careful observations with the new 100-inch telescope, Hubble disc ...
... Hubble studied the Andromeda Nebula, which had been thought by many, including Shapley, to be a gas cloud within the Milky Way. The word nebula comes from the Latin nubes, or “cloud,” denoting the fuzzy appearance of these objects. By careful observations with the new 100-inch telescope, Hubble disc ...
PSC100 Transparant Replacement for Chapter 8 Measurement of
... * Determine two light sources are similar in brightness. Similar spectra class should mean that the two stars have about the same intrinsic brightness. Variable stars have flash rates that tell their luminosity. 5th brightest galaxy in any cluster assumed to have about the same absolute magnitude. S ...
... * Determine two light sources are similar in brightness. Similar spectra class should mean that the two stars have about the same intrinsic brightness. Variable stars have flash rates that tell their luminosity. 5th brightest galaxy in any cluster assumed to have about the same absolute magnitude. S ...
Astronomy In the News Parallax Class demos: Parallax
... a) 2 pc = 6.5 light years b) 20 pc = 65 light years c) 200 pc = 650 light years ...
... a) 2 pc = 6.5 light years b) 20 pc = 65 light years c) 200 pc = 650 light years ...
Ay 122a Fall 2012 – HOMEWORK #1
... as it transits through the local meridian, midnight local time. (a) What is the local siderial time? (b) What day of the year is it? (c) What is the approximate universal time (assume that you are in California)? (d) Can you do this from Palomar anyway (Palomar’s latitude is +33◦ 210 2100 (e) What i ...
... as it transits through the local meridian, midnight local time. (a) What is the local siderial time? (b) What day of the year is it? (c) What is the approximate universal time (assume that you are in California)? (d) Can you do this from Palomar anyway (Palomar’s latitude is +33◦ 210 2100 (e) What i ...
Focus On Middle School Astronomy Student
... of stars that can be seen from the northern hemisphere from December through March. Orion has a “belt” of three bright stars in a straight row. Once the “belt” is located, it is easy to find the “club” and “shield” by looking for neighboring stars. ...
... of stars that can be seen from the northern hemisphere from December through March. Orion has a “belt” of three bright stars in a straight row. Once the “belt” is located, it is easy to find the “club” and “shield” by looking for neighboring stars. ...
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.