Astronomical Knowledge Questionnaire (Teacher
... in summer there are few clouds which means the light coming from the Sun is stronger. The Earth’s tilted axis means that one hemisphere has more direct sunlight and longer days making it summer while the other hemisphere experiences winter. The Sun moves to make one side of the Earth hot for six ...
... in summer there are few clouds which means the light coming from the Sun is stronger. The Earth’s tilted axis means that one hemisphere has more direct sunlight and longer days making it summer while the other hemisphere experiences winter. The Sun moves to make one side of the Earth hot for six ...
talk / PPT / 1.6 MB
... Milky Way compared to External discs Where does the Milky Way lie on the Tully-Fisher relation? Pretty much within the (1-sigma) scatter. ...
... Milky Way compared to External discs Where does the Milky Way lie on the Tully-Fisher relation? Pretty much within the (1-sigma) scatter. ...
Slide 1
... be sufficiently stiff to support 2-M neutron stars and at the same time sufficiently soft to make neutron stars with moderate radii n the canonical mass range. This balance appears to be difficult to ...
... be sufficiently stiff to support 2-M neutron stars and at the same time sufficiently soft to make neutron stars with moderate radii n the canonical mass range. This balance appears to be difficult to ...
Supernova Stalking - Susanna Kumlien Reportage
... investigated more thoroughly. What type of star gives birth to what kind of supernova? Photos taken before and after the explosion will disclose yet unseen data. The method of image subtracting is being used, a process where digital numeric values of a picture are subtracted from the previous image, ...
... investigated more thoroughly. What type of star gives birth to what kind of supernova? Photos taken before and after the explosion will disclose yet unseen data. The method of image subtracting is being used, a process where digital numeric values of a picture are subtracted from the previous image, ...
pptx
... Luminosity of main sequence stars is determined by mass Main sequence is a mass sequence (bright hot stars are more massive, cool faint stars are less massive) 10 times as massive 10000 times brighter! ...
... Luminosity of main sequence stars is determined by mass Main sequence is a mass sequence (bright hot stars are more massive, cool faint stars are less massive) 10 times as massive 10000 times brighter! ...
star signs - Museum of the Rockies
... Alternating between a narrator and various storytellers, the first half of this show is a recorded explanation of the constellations and the way different cultures viewed the night sky. The importance of the night sky to ancient Babylonians and Greeks is described in turn. The significance of the zo ...
... Alternating between a narrator and various storytellers, the first half of this show is a recorded explanation of the constellations and the way different cultures viewed the night sky. The importance of the night sky to ancient Babylonians and Greeks is described in turn. The significance of the zo ...
Hubble Space Telescope Image
... The Universe is filled with these star systems which themselves cluster together into larger systems. Earth & Space Science March 2015 ...
... The Universe is filled with these star systems which themselves cluster together into larger systems. Earth & Space Science March 2015 ...
Astro-MilkyWay
... measurement of the distances to the globular clusters? a. The Sun is far from the center of the Milky Way. b. The Sun is near the center of the Milky Way. c. A period-luminosity relationship also exists for RR Lyrae variable stars. d. Globular clusters have 50,000 to 1,000,000 stars. e. Open cluster ...
... measurement of the distances to the globular clusters? a. The Sun is far from the center of the Milky Way. b. The Sun is near the center of the Milky Way. c. A period-luminosity relationship also exists for RR Lyrae variable stars. d. Globular clusters have 50,000 to 1,000,000 stars. e. Open cluster ...
Orion the Hunter
... Hunter. Its brightest stars form one of the best known celestial shapes, which is visible even from cities. The plane of the Milky Way clips the northeast corner of the constellation and manifests itself as a featureless, hazy band through the neighboring constellations of Gemini and Monoceros. Or ...
... Hunter. Its brightest stars form one of the best known celestial shapes, which is visible even from cities. The plane of the Milky Way clips the northeast corner of the constellation and manifests itself as a featureless, hazy band through the neighboring constellations of Gemini and Monoceros. Or ...
Spiral structure of the Third Galactic Quadrant and the solution to the
... Fig. 1) has been taken as strong evidence for the existence of the CMa galaxy (Bellazzini et al. 2004; Dinescu et al. 2005; Martı́nez-Delgado et al. 2005). The BP has been modelled and interpreted as the last burst of star formation in that galaxy 1-2 Gyr ago (which, given that it is a 1-2 Gyr popul ...
... Fig. 1) has been taken as strong evidence for the existence of the CMa galaxy (Bellazzini et al. 2004; Dinescu et al. 2005; Martı́nez-Delgado et al. 2005). The BP has been modelled and interpreted as the last burst of star formation in that galaxy 1-2 Gyr ago (which, given that it is a 1-2 Gyr popul ...
Review: How does a star*s mass determine its life story?
... — Use orbital properties of companion — Measure velocity and distance of orbiting gas • It’s a black hole if it’s not a star and its mass exceeds the neutron star limit (~3 MSun). ...
... — Use orbital properties of companion — Measure velocity and distance of orbiting gas • It’s a black hole if it’s not a star and its mass exceeds the neutron star limit (~3 MSun). ...
Death of Massive Stars
... The Earth completely? • Depends on the mass of the Earth and your distance from the center of the Earth. • At Earth’s surface: 25,000 mph (11km/s) • From the top of a 1000 mile high tower, 22,000 mph (10km/s) • From the surface of the Sun? (Mass 1MSUN, radius 700,000km): 1,400,000 mph (620km/s) • Fr ...
... The Earth completely? • Depends on the mass of the Earth and your distance from the center of the Earth. • At Earth’s surface: 25,000 mph (11km/s) • From the top of a 1000 mile high tower, 22,000 mph (10km/s) • From the surface of the Sun? (Mass 1MSUN, radius 700,000km): 1,400,000 mph (620km/s) • Fr ...
Exercises
... (a) Calculate the total energy of the Sun assuming that the density is constant, i.e. using the equation for potential energy Egr = -3/5 GM2 /R. In later phases, stars like the Sun become red giants, with R ≈ 100R . What would be the total energy, if the giant had constant density. Assume that the ...
... (a) Calculate the total energy of the Sun assuming that the density is constant, i.e. using the equation for potential energy Egr = -3/5 GM2 /R. In later phases, stars like the Sun become red giants, with R ≈ 100R . What would be the total energy, if the giant had constant density. Assume that the ...
DoAr21_AAS2005 - Astronomy at Swarthmore College
... PMS stars have stronger and harder x-ray emission than cool mainsequence stars. They also exhibit significant x-ray time variability. Is PMS x-ray activity similar in origin to solar-type x-ray activity (alpha-omega dynamo driven)? If so, why is it stronger? Is it connected to accretion? ...
... PMS stars have stronger and harder x-ray emission than cool mainsequence stars. They also exhibit significant x-ray time variability. Is PMS x-ray activity similar in origin to solar-type x-ray activity (alpha-omega dynamo driven)? If so, why is it stronger? Is it connected to accretion? ...
WHERE DO ELEMENTS COME FROM?
... • Alpher and Gamow also predicted that the heat present during the first few minutes is still present in the universe • The universe should have now expanded and be on average only a few Kelvins hot • The wave length of this radiation should be in the range of microwaves ...
... • Alpher and Gamow also predicted that the heat present during the first few minutes is still present in the universe • The universe should have now expanded and be on average only a few Kelvins hot • The wave length of this radiation should be in the range of microwaves ...
Open Houses at the Campus Observatory Astronomical Horizons Lecture
... The sun becomes degenerate The sun loses too much mass as a planetary nebula It takes too long to burn neon. ...
... The sun becomes degenerate The sun loses too much mass as a planetary nebula It takes too long to burn neon. ...
Astronomy 252: Short Project 2 Stellar Spectra: Their Classification
... stars. The beautiful thing about spectral classification is that one does not really need to know anything about stellar astrophysics to classify a spectrum. Think of spectral classification as simply an exercise in pattern matching. What you want to do is to "bracket" the unknown spectrum between t ...
... stars. The beautiful thing about spectral classification is that one does not really need to know anything about stellar astrophysics to classify a spectrum. Think of spectral classification as simply an exercise in pattern matching. What you want to do is to "bracket" the unknown spectrum between t ...
Review: How does a star`s mass determine its life story?
... White dwarf supernova: A white dwarf in close binary system reaches the white dwarf mass limit, causing an explosion. Carbon fusion may re-ignite for a brief time for the explosion. The Energy released is enough to destroy the star completely, an there is NO neutron star left behind. ...
... White dwarf supernova: A white dwarf in close binary system reaches the white dwarf mass limit, causing an explosion. Carbon fusion may re-ignite for a brief time for the explosion. The Energy released is enough to destroy the star completely, an there is NO neutron star left behind. ...
Perseus (constellation)
Perseus, named after the Greek mythological hero Perseus, is a constellation in the northern sky. It was one of 48 listed by the 2nd-century astronomer Ptolemy and among the 88 modern constellations defined by the International Astronomical Union (IAU). It is located in the northern celestial hemisphere near several other constellations named after legends surrounding Perseus, including Andromeda to the west and Cassiopeia to the north. Perseus is also bordered by Aries and Taurus to the south, Auriga to the east, Camelopardalis to the north, and Triangulum to the west.The galactic plane of the Milky Way passes through Perseus but is mostly obscured by molecular clouds. The constellation's brightest star is the yellow-white supergiant Alpha Persei (also called Mirfak), which shines at magnitude 1.79. It and many of the surrounding stars are members of an open cluster known as the Alpha Persei Cluster. The best-known star, however, is Algol (Beta Persei), linked with ominous legends because of its variability, which is noticeable to the naked eye. Rather than being an intrinsically variable star, it is an eclipsing binary. Other notable star systems in Perseus include X Persei, a binary system containing a neutron star, and GK Persei, a nova that peaked at magnitude 0.2 in 1901. The Double Cluster, comprising two open clusters quite near each other in the sky, was known to the ancient Chinese. The constellation gives its name to the Perseus Cluster (Abell 426), a massive galaxy cluster located 250 million light-years from Earth. It hosts the radiant of the annual Perseids meteor shower—one of the most prominent meteor showers in the sky.