Reader`s Theater Our Closest Star
... strong enough to hold all of the parts of this system together. Is it any wonder the system is named after me? I am a star, your closest star. I may be millions of times closer to you than other stars, but I am still very far away. It would take a jet plane nineteen years to reach me. But, of course ...
... strong enough to hold all of the parts of this system together. Is it any wonder the system is named after me? I am a star, your closest star. I may be millions of times closer to you than other stars, but I am still very far away. It would take a jet plane nineteen years to reach me. But, of course ...
The Sun, Stars, and Beyond
... • The most common is the elliptical galaxy, shaped sort of like a big egg. • There are spiral and barred spiral galaxies, • Irregularly shaped galaxies also exist, though fewer in number. • A galaxy’s shape is determined by its rate of spin, and if it has been subject to any collisions or mergers. • ...
... • The most common is the elliptical galaxy, shaped sort of like a big egg. • There are spiral and barred spiral galaxies, • Irregularly shaped galaxies also exist, though fewer in number. • A galaxy’s shape is determined by its rate of spin, and if it has been subject to any collisions or mergers. • ...
star - TeacherWeb
... Light from stars that are moving toward the Earth is shifted slightly toward the blue end of the spectrum. When a source of light (like a star) is stationary, the wavelengths of light remain the same distance apart. When a source of light is moving toward you, the wavelengths of light get closer tog ...
... Light from stars that are moving toward the Earth is shifted slightly toward the blue end of the spectrum. When a source of light (like a star) is stationary, the wavelengths of light remain the same distance apart. When a source of light is moving toward you, the wavelengths of light get closer tog ...
distance to the centre of the Milky Way.
... From measured brightnesses of some of the stars in the globular clusters (in particular, by studying some variable stars of a characteristic luminosity), Shapley was able to derive the distances to many of the clusters. ...
... From measured brightnesses of some of the stars in the globular clusters (in particular, by studying some variable stars of a characteristic luminosity), Shapley was able to derive the distances to many of the clusters. ...
Measuring Stars
... Hydrogen Spectrum Star B is A) Made of two kinds of hydrogen B) Moving away from us AND moving towards us C) Actually two stars moving at different speeds ...
... Hydrogen Spectrum Star B is A) Made of two kinds of hydrogen B) Moving away from us AND moving towards us C) Actually two stars moving at different speeds ...
Constellation ProjectConstellation Project(es)
... 11. If you selected a constellation that is not in the “Stories of the Constellation” research on the internet your constellations story. If you still can not find it, write your own story for your ...
... 11. If you selected a constellation that is not in the “Stories of the Constellation” research on the internet your constellations story. If you still can not find it, write your own story for your ...
Chapter 12: Measuring the Properties of Stars
... 1. An astrometric binary is an orbiting pair of stars in which the motion of one of the stars reveals the presence of the other. 2. A composite spectrum binary is a binary star system with stars having spectra different enough to distinguish them from one another. 12-6 Stellar Masses and Sizes from ...
... 1. An astrometric binary is an orbiting pair of stars in which the motion of one of the stars reveals the presence of the other. 2. A composite spectrum binary is a binary star system with stars having spectra different enough to distinguish them from one another. 12-6 Stellar Masses and Sizes from ...
Mass
... Because the star is so far away, the scientist could not have the time to receive the radio signals from such a planet. B Because the star is so close that we should have received radio signals from the planet years ago. C Because the radio signals cannot penetrate the Earth’s atmosphere from ...
... Because the star is so far away, the scientist could not have the time to receive the radio signals from such a planet. B Because the star is so close that we should have received radio signals from the planet years ago. C Because the radio signals cannot penetrate the Earth’s atmosphere from ...
Astronomy_Stars_n_Galaxies_PowerPoint
... that the light given off by a star or galaxy gets “stretched” if it is moving away from us. This causes the light being given off to have a longer wavelength and the object to appear redder than it really is. This is called the red shift. Using Hubble’s idea, astronomers found that all distant galax ...
... that the light given off by a star or galaxy gets “stretched” if it is moving away from us. This causes the light being given off to have a longer wavelength and the object to appear redder than it really is. This is called the red shift. Using Hubble’s idea, astronomers found that all distant galax ...
Interpreting the HR diagram of stellar clusters
... There are very massive, hot, blue stars at the top-left of the HR diagram, as well as low-mass, cool, red stars at the bottom-right. Now, in real life, the stars in a giant molecular cloud don't all finish contracting and begin to fuse hydrogen simultaneously; there is always a small spread of seve ...
... There are very massive, hot, blue stars at the top-left of the HR diagram, as well as low-mass, cool, red stars at the bottom-right. Now, in real life, the stars in a giant molecular cloud don't all finish contracting and begin to fuse hydrogen simultaneously; there is always a small spread of seve ...
Black Hole
... It took almost eight months to fade away from the sky. It sparkled like a star in the sky. Today we know it was a `Supernova'. ...
... It took almost eight months to fade away from the sky. It sparkled like a star in the sky. Today we know it was a `Supernova'. ...
The Death of a Low Mass Star
... – looking through a greater depth of material at the edges Core of “dead” star ...
... – looking through a greater depth of material at the edges Core of “dead” star ...
Why Study Binary Stars?
... The amount of light lost depends on eclipsed area & temperature The area covered at each minimum is the same Depth of the minimum depends on eclipsed star’s temperature Primary eclipse is always when the hotter star is behind the cooler star ...
... The amount of light lost depends on eclipsed area & temperature The area covered at each minimum is the same Depth of the minimum depends on eclipsed star’s temperature Primary eclipse is always when the hotter star is behind the cooler star ...
Pulsars - Chabot College
... Essay Questions for the exam… (a) What is a pulsar? Where does it get its ...
... Essay Questions for the exam… (a) What is a pulsar? Where does it get its ...
Neutron Star - Perry Local Schools
... of 1.4 to 3 solar masses, the remnant can become a neutron star. – If the leftover core has a mass that is greater than three solar masses, it will collapse to form a black ...
... of 1.4 to 3 solar masses, the remnant can become a neutron star. – If the leftover core has a mass that is greater than three solar masses, it will collapse to form a black ...
O star
... The calibration of the full H-R diagram: clusters to the rescue! • Many stars of many spectral types have examples close enough to get distance from parallaxes. • Some types of stars are rare, e.g., O stars, M supergiants, there are no nearby examples, and hence no parallax ...
... The calibration of the full H-R diagram: clusters to the rescue! • Many stars of many spectral types have examples close enough to get distance from parallaxes. • Some types of stars are rare, e.g., O stars, M supergiants, there are no nearby examples, and hence no parallax ...
Cygnus (constellation)
Cygnus /ˈsɪɡnəs/ is a northern constellation lying on the plane of the Milky Way, deriving its name from the Latinized Greek word for swan. The swan is one of the most recognizable constellations of the northern summer and autumn, it features a prominent asterism known as the Northern Cross (in contrast to the Southern Cross). Cygnus was among the 48 constellations listed by the 2nd century astronomer Ptolemy, and it remains one of the 88 modern constellations.Cygnus contains Deneb, one of the brightest stars in the night sky and one corner of the Summer Triangle, as well as some notable X-ray sources and the giant stellar association of Cygnus OB2. One of the stars of this association, NML Cygni, is one of the largest stars currently known. The constellation is also home to Cygnus X-1, a distant X-ray binary containing a supergiant and unseen massive companion that was the first object widely held to be a black hole. Many star systems in Cygnus have known planets as a result of the Kepler Mission observing one patch of the sky, the patch is the area around Cygnus. In addition, most of the eastern part of Cygnus is dominated by the Hercules–Corona Borealis Great Wall, a giant galaxy filament that is the largest known structure in the observable universe; covering most of the northern sky.