Astronomy 242: Review Questions #1 Distributed: February 10
... 12. You observe a sample of Cepheid variable stars in a nearby galaxy. Plotting the average apparent K-band magnitude of each one against the period of pulsation yields Fig. 3. The straight line, a least-squares fit to the data, has the equation mK = 16.40 − 3.53 log(P/day). (a) Does it seem reasona ...
... 12. You observe a sample of Cepheid variable stars in a nearby galaxy. Plotting the average apparent K-band magnitude of each one against the period of pulsation yields Fig. 3. The straight line, a least-squares fit to the data, has the equation mK = 16.40 − 3.53 log(P/day). (a) Does it seem reasona ...
Chapter 13 Notes – The Deaths of Stars
... Sun will expand to a red giant in ______________ billion years Expands to ______________ radius Earth will then be ___________________ Sun MAY form a ________________ nebula (but uncertain) Sun’s C, O core will become a ______________ dwarf VIII. The Deaths of Massive Stars: Supernovae F ...
... Sun will expand to a red giant in ______________ billion years Expands to ______________ radius Earth will then be ___________________ Sun MAY form a ________________ nebula (but uncertain) Sun’s C, O core will become a ______________ dwarf VIII. The Deaths of Massive Stars: Supernovae F ...
Startalk
... A big glowing ball of gas! Contains mainly H and He They have a core that is dense and super hot! Nuclear fusion is the source of their energy! ...
... A big glowing ball of gas! Contains mainly H and He They have a core that is dense and super hot! Nuclear fusion is the source of their energy! ...
Codes of Life
... start to use helium as a fuel producing carbon. It also begins burning hydrogen in its atmosphere and will expand 100 times to become the red giant • When this happens to our Sun (in about 4 billion years) all inner planets and the Earth will be incinerated. ...
... start to use helium as a fuel producing carbon. It also begins burning hydrogen in its atmosphere and will expand 100 times to become the red giant • When this happens to our Sun (in about 4 billion years) all inner planets and the Earth will be incinerated. ...
Ch.10 Stellar old age
... Core of helium is supported by electron degeneracy pressure When He ‘ignites’, whole core is ready to fuse He into C ...
... Core of helium is supported by electron degeneracy pressure When He ‘ignites’, whole core is ready to fuse He into C ...
What are stars?
... Compare the development of a less-massive star with that of a more-massive star. ___________________________________________________________________ ___________________________________________________________________ ___________________________________________________________________ _______________ ...
... Compare the development of a less-massive star with that of a more-massive star. ___________________________________________________________________ ___________________________________________________________________ ___________________________________________________________________ _______________ ...
Chapter 8, Lesson 4, 2nd Packet, pdf
... Compare the development of a less-massive star with that of a more-massive star. ___________________________________________________________________ ___________________________________________________________________ ___________________________________________________________________ _______________ ...
... Compare the development of a less-massive star with that of a more-massive star. ___________________________________________________________________ ___________________________________________________________________ ___________________________________________________________________ _______________ ...
Main Sequence Star
... a) Size of giants depends on the initial mass b) Could be a super red giant like Betelgeuse ...
... a) Size of giants depends on the initial mass b) Could be a super red giant like Betelgeuse ...
Review Game
... 38) An object compacted to such a small size that light cannot escape from its gravitational field is called a: 39) The spherical surface of space which defines the "surface" of a black hole is the: 40) White dwarfs, like Sirius B, would be found to the ________ on the H-R diagram. 41) A red supergi ...
... 38) An object compacted to such a small size that light cannot escape from its gravitational field is called a: 39) The spherical surface of space which defines the "surface" of a black hole is the: 40) White dwarfs, like Sirius B, would be found to the ________ on the H-R diagram. 41) A red supergi ...
Astronomical Terms - Crossroads Academy
... circumpolar stars…stars that never set from where you observe them over an entire year constellation…88 sections of the sky including star arrangements with names mostly derived from ancient astronomy…the study of the celestial objects asterism…group of stars Great Bear (stars — Dubhe, Merak, Mizar, ...
... circumpolar stars…stars that never set from where you observe them over an entire year constellation…88 sections of the sky including star arrangements with names mostly derived from ancient astronomy…the study of the celestial objects asterism…group of stars Great Bear (stars — Dubhe, Merak, Mizar, ...
Mr - White Plains Public Schools
... There is a relationship between the temperatures of stars and how bright they are (luminosity). In general, the hotter a star the brighter. This is not always true though. For example, Polaris is the same temperature as our Sun, but is around 4000X brighter. This difference is due to the mass and si ...
... There is a relationship between the temperatures of stars and how bright they are (luminosity). In general, the hotter a star the brighter. This is not always true though. For example, Polaris is the same temperature as our Sun, but is around 4000X brighter. This difference is due to the mass and si ...
Test#3
... a) they rotate slowly, b) they are a few km in radius c) they have large magnetic fields, d) some of them are observed to be pulsars 28. Which of the following objects can rotate a thousand times per second without being torn apart? a) white dwarf, b) main sequence star, c) red giant, d) neutron sta ...
... a) they rotate slowly, b) they are a few km in radius c) they have large magnetic fields, d) some of them are observed to be pulsars 28. Which of the following objects can rotate a thousand times per second without being torn apart? a) white dwarf, b) main sequence star, c) red giant, d) neutron sta ...
The Life Cycle of Stars
... For stars tens of times more massive than the sun, the outer layers of the star explode outwards (supernova: a stellar explosion that occurs at the end of a massive star’s life) After the explosion, the core left behind becomes a neutron star (the gravity of a neutron star is 300000times that of Ear ...
... For stars tens of times more massive than the sun, the outer layers of the star explode outwards (supernova: a stellar explosion that occurs at the end of a massive star’s life) After the explosion, the core left behind becomes a neutron star (the gravity of a neutron star is 300000times that of Ear ...
Monday, April 15
... • Then do the following Gedankenexperiment: – In your mind, put the star from its actual position to a position 10 pc away – If a star is actually closer than 10pc, its absolute magnitude will be a bigger number, i.e. it is intrinsically dimmer than it appears – If a star is farther than 10pc, its a ...
... • Then do the following Gedankenexperiment: – In your mind, put the star from its actual position to a position 10 pc away – If a star is actually closer than 10pc, its absolute magnitude will be a bigger number, i.e. it is intrinsically dimmer than it appears – If a star is farther than 10pc, its a ...
Supernova
... • The nuclei from fusion are separated from their electrons. – Filled fermi states with degenerate electrons – Provides opposing force to gravity • The energy of contraction blows off outer layers of star. ...
... • The nuclei from fusion are separated from their electrons. – Filled fermi states with degenerate electrons – Provides opposing force to gravity • The energy of contraction blows off outer layers of star. ...
HR Diagram Activity
... Materials: Colored pencils (red, orange, yellow, blue) Procedure: 1. Review the star data chart below. Note that the sun, which is used as a standard of brightness, is given a value of 1. The brightness given for each other star shows how that star compares with the sun. 2. Using an “X” as a plot po ...
... Materials: Colored pencils (red, orange, yellow, blue) Procedure: 1. Review the star data chart below. Note that the sun, which is used as a standard of brightness, is given a value of 1. The brightness given for each other star shows how that star compares with the sun. 2. Using an “X” as a plot po ...
How Bright is that Star?
... A 1st magnitude star is 100x brighter than a “6th ” Each order of magnitude is therefore 2.15 times brighter than the one below it. Magnitude is now given in decimal form. Deneb now rates a 1.26, and Betelgeuse rates .87. Hipparchus underestimated how bright the brightest were, so now we even use ne ...
... A 1st magnitude star is 100x brighter than a “6th ” Each order of magnitude is therefore 2.15 times brighter than the one below it. Magnitude is now given in decimal form. Deneb now rates a 1.26, and Betelgeuse rates .87. Hipparchus underestimated how bright the brightest were, so now we even use ne ...
Constellations and Planets in the Night Sky
... Planets are closer to us than stars and they are in constant motion as they move around, or orbit, the sun. Because of this, they can be seem in different locations in the night sky in relation to the constellations. ...
... Planets are closer to us than stars and they are in constant motion as they move around, or orbit, the sun. Because of this, they can be seem in different locations in the night sky in relation to the constellations. ...
Chapter 1 Vocabulary – The Puzzled of Matter
... Absorption Lines – a set of dark lines that show frequencies at which light has been absorbed from a star’s bright spectrum H-R Diagram – the Hertxsprung-Russell diagram, a graph of the surface temperature versus absolute brightness of a sample of stars Star Life Cycle Nebula – a large cloud of gas ...
... Absorption Lines – a set of dark lines that show frequencies at which light has been absorbed from a star’s bright spectrum H-R Diagram – the Hertxsprung-Russell diagram, a graph of the surface temperature versus absolute brightness of a sample of stars Star Life Cycle Nebula – a large cloud of gas ...
PowerPoint Presentation - Welcome to Modern Astronomy Fall 2003
... who I am, who you are • This should be the most interesting course you take in college • National Solar Observatory ...
... who I am, who you are • This should be the most interesting course you take in college • National Solar Observatory ...
Corvus (constellation)
Corvus is a small constellation in the Southern Celestial Hemisphere. Its name comes from the Latin word ""raven"" or ""crow"". It includes only 11 stars with brighter than 4.02 magnitudes. One of the 48 constellations listed by the 2nd-century astronomer Ptolemy, it remains one of the 88 modern constellations. The four brightest stars, Gamma, Delta, Epsilon, and Beta Corvi from a distinctive quadrilateral in the night sky. The young star Eta Corvi has been found to have two debris disks.