Volcanoes and Igneous Activity Earth - Chapter 4
... Dissemination or sale of any part of this work (including on the World Wide Web) will destroy the integrity of the work and is not permitted. The work and materials from it should never be made available to students except by instructors using the accompanying text in their classes. All recipients o ...
... Dissemination or sale of any part of this work (including on the World Wide Web) will destroy the integrity of the work and is not permitted. The work and materials from it should never be made available to students except by instructors using the accompanying text in their classes. All recipients o ...
Galactic Structure
... different elemental ratios than do field halo stars… Milky Way field stars ...
... different elemental ratios than do field halo stars… Milky Way field stars ...
DTU_9e_ch13
... A pulsar is a rapidly rotating neutron star with a powerful magnetic field that makes it a source of periodic radio and other electromagnetic pulses. Energy pours out of the polar regions of the neutron star in intense beams that sweep across the sky. ...
... A pulsar is a rapidly rotating neutron star with a powerful magnetic field that makes it a source of periodic radio and other electromagnetic pulses. Energy pours out of the polar regions of the neutron star in intense beams that sweep across the sky. ...
Stars, Galaxies & Universe
... Size- Giant, main sequence, and dwarf Temperature- blue=hot; red=cooler Brightness- apparent brightness and absolute magnitude HR diagram shows temperature, brightness, color of stars and where the star is in its life cycle. Used to graph the surface temperature (x-axis) vs. brightness (yaxis) Hotte ...
... Size- Giant, main sequence, and dwarf Temperature- blue=hot; red=cooler Brightness- apparent brightness and absolute magnitude HR diagram shows temperature, brightness, color of stars and where the star is in its life cycle. Used to graph the surface temperature (x-axis) vs. brightness (yaxis) Hotte ...
Feb 2017 - What`s Out Tonight?
... well liked for its blue & gold colors. Ptolemaeus magnitude +11. The second closest star visible to Alphonsus the naked eye is Sirius at 8.6 ly followed by Epsilon Moon (e) Eridani at 10.5 ly and Procyon at 11.4 ly. There Tycho Starting from New Moon, the Moon cycles through are several stars closer ...
... well liked for its blue & gold colors. Ptolemaeus magnitude +11. The second closest star visible to Alphonsus the naked eye is Sirius at 8.6 ly followed by Epsilon Moon (e) Eridani at 10.5 ly and Procyon at 11.4 ly. There Tycho Starting from New Moon, the Moon cycles through are several stars closer ...
Back to basics: naked-eye astronomical observation
... wide as possible (dark adapted). This can easily be seen with a red bulb in a room if pupils are paired up looking into each other’s eyes and then the white light is turned on. Do this in advance of your observing session and they will appreciate why they should bring a red torch (or a normal one wi ...
... wide as possible (dark adapted). This can easily be seen with a red bulb in a room if pupils are paired up looking into each other’s eyes and then the white light is turned on. Do this in advance of your observing session and they will appreciate why they should bring a red torch (or a normal one wi ...
Chapter 27.1
... How is a star’s surface temperature and composition determined? Explain why, to an observer on earth, stars appear to move. Describe the ways distances from the earth to the stars are measured. Explain the difference between absolute and apparent magnitude. ...
... How is a star’s surface temperature and composition determined? Explain why, to an observer on earth, stars appear to move. Describe the ways distances from the earth to the stars are measured. Explain the difference between absolute and apparent magnitude. ...
12 Introduction to Cepheid Variable Stars Exercise
... distance to the bulb. This can be applied to stars, if you determine the apparent magnitude of the star and you know the absolute magnitude then you can calculate the distance to the star. Miss Henrietta Leavitt (1868 - 1921), working at the Harvard Observatory, determined the apparent magnitude and ...
... distance to the bulb. This can be applied to stars, if you determine the apparent magnitude of the star and you know the absolute magnitude then you can calculate the distance to the star. Miss Henrietta Leavitt (1868 - 1921), working at the Harvard Observatory, determined the apparent magnitude and ...
Teachers Notes - Edinburgh International Science Festival
... Observing the Universe Due to the vast distances between Earth and our neighbouring planets, stars and galaxies, the main way that scientists explore our universe is by observing and detecting light with telescopes. Light is emitted and reflected off many objects in space. This light contains inform ...
... Observing the Universe Due to the vast distances between Earth and our neighbouring planets, stars and galaxies, the main way that scientists explore our universe is by observing and detecting light with telescopes. Light is emitted and reflected off many objects in space. This light contains inform ...
The birth and life of stars
... Star formation begins when gravitational attraction causes clumps of gas and dust, called protostars, to coalesce in Bok globules within a giant molecular cloud. As a protostar contracts, its matter begins to heat and glow. When the contraction slows down, the protostar becomes a pre–main-sequence ...
... Star formation begins when gravitational attraction causes clumps of gas and dust, called protostars, to coalesce in Bok globules within a giant molecular cloud. As a protostar contracts, its matter begins to heat and glow. When the contraction slows down, the protostar becomes a pre–main-sequence ...
Star Evolution
... They leave the main sequence and become red giants when the core hydrogen is depleted” ...
... They leave the main sequence and become red giants when the core hydrogen is depleted” ...
1” “Sky-Notes” of the Open University Astronomy Club. April 2005
... NGC2903 (8.9) sg. A spiral galaxy inclined to our line of sight. One of the brightest galaxies in Leo it is surprisingly not a Messier object. NGC3190 (11.0) sg and NGC3193 (10.9) eg. Pair of galaxies located mid-way between and . NGC3226 (11.4) and NGC3227 (10.8) about 1o east of form a close ...
... NGC2903 (8.9) sg. A spiral galaxy inclined to our line of sight. One of the brightest galaxies in Leo it is surprisingly not a Messier object. NGC3190 (11.0) sg and NGC3193 (10.9) eg. Pair of galaxies located mid-way between and . NGC3226 (11.4) and NGC3227 (10.8) about 1o east of form a close ...
Stellar Spire in the Eagle Nebula
... this object is actually a billowing tower of cold gas and dust rising from a stellar nursery called the Eagle Nebula. The soaring tower is 9.5 light-years or about 57 trillion miles high, about twice the distance from our Sun to the next nearest star. Stars in the Eagle Nebula are born in clouds of ...
... this object is actually a billowing tower of cold gas and dust rising from a stellar nursery called the Eagle Nebula. The soaring tower is 9.5 light-years or about 57 trillion miles high, about twice the distance from our Sun to the next nearest star. Stars in the Eagle Nebula are born in clouds of ...
DO NOW - PBworks
... The student is expected to explore how different wavelengths of the electromagnetic spectrum such as light and radio waves are used to gain information about distances and properties of components in the universe. ...
... The student is expected to explore how different wavelengths of the electromagnetic spectrum such as light and radio waves are used to gain information about distances and properties of components in the universe. ...
4. Survey Observations
... earlier for the same star to be on your meridian – each month, you must observe 2 hours earlier for the same star to be on you meridian (a given RA is on your meridian 2 hours earlier each month) • Thus, the airmass of a star changes through the year as the star becomes easier or harder to observe • ...
... earlier for the same star to be on your meridian – each month, you must observe 2 hours earlier for the same star to be on you meridian (a given RA is on your meridian 2 hours earlier each month) • Thus, the airmass of a star changes through the year as the star becomes easier or harder to observe • ...
BAS - Monthly Sky Guide
... The constellation Lupus, “The Wolf”, sits near the half-man half-horse warrior beast the Centaur and mythology suggests a fight to the death between the two is underway in the sky. Lupus is also not far from Libra and the central bulge region of our Milky Way Galaxy – this means it is a good place ...
... The constellation Lupus, “The Wolf”, sits near the half-man half-horse warrior beast the Centaur and mythology suggests a fight to the death between the two is underway in the sky. Lupus is also not far from Libra and the central bulge region of our Milky Way Galaxy – this means it is a good place ...
Mar 2017 - What`s Out Tonight?
... well liked for its blue & gold colors. Ptolemaeus magnitude +11. The second closest star visible to Alphonsus the naked eye is Sirius at 8.6 ly followed by Epsilon Moon (e) Eridani at 10.5 ly and Procyon at 11.4 ly. There Tycho Starting from New Moon, the Moon cycles through are several stars closer ...
... well liked for its blue & gold colors. Ptolemaeus magnitude +11. The second closest star visible to Alphonsus the naked eye is Sirius at 8.6 ly followed by Epsilon Moon (e) Eridani at 10.5 ly and Procyon at 11.4 ly. There Tycho Starting from New Moon, the Moon cycles through are several stars closer ...
Stellar Evolution
... • Mass of Sun • Radius of Earth • Hot as Sun’s core • A million times denser than lead • Slowly cool off ...
... • Mass of Sun • Radius of Earth • Hot as Sun’s core • A million times denser than lead • Slowly cool off ...
Chapter 19 Star Formation
... “distorted way: In fact the clouds are usually much more irregular than shown in this textbook illustration. (Note: all the colorful emission line nebulae shown in this chapter are just this same molecular gas after a massive stars has started pouring out photons. ...
... “distorted way: In fact the clouds are usually much more irregular than shown in this textbook illustration. (Note: all the colorful emission line nebulae shown in this chapter are just this same molecular gas after a massive stars has started pouring out photons. ...
Lyra
Lyra (/ˈlaɪərə/; Latin for lyre, from Greek λύρα) is a small constellation. It is one of 48 listed by the 2nd century astronomer Ptolemy, and is one of the 88 constellations recognized by the International Astronomical Union. Lyra was often represented on star maps as a vulture or an eagle carrying a lyre, and hence sometimes referred to as Aquila Cadens or Vultur Cadens. Beginning at the north, Lyra is bordered by Draco, Hercules, Vulpecula, and Cygnus. Lyra is visible from the northern hemisphere from spring through autumn, and nearly overhead, in temperate latitudes, during the summer months. From the southern hemisphere, it is visible low in the northern sky during the winter months.The lucida or brightest star—and one of the brightest stars in the sky—is the white main sequence star Vega, a corner of the Summer Triangle. Beta Lyrae is the prototype of a class of stars known as Beta Lyrae variables, binary stars so close to each other that they become egg-shaped and material flows from one to the other. Epsilon Lyrae, known informally as the Double Double, is a complex multiple star system. Lyra also hosts the Ring Nebula, the second-discovered and best-known planetary nebula.