Superwind - The University of Sydney
... they are driven by minute dust grains, which form in the atmosphere of the star and absorb its light. The star light pushes the dust grains (silicates) away from the star. However, models show that this mechanism does not work well. The dust grains become too hot, and evaporate before they can be pu ...
... they are driven by minute dust grains, which form in the atmosphere of the star and absorb its light. The star light pushes the dust grains (silicates) away from the star. However, models show that this mechanism does not work well. The dust grains become too hot, and evaporate before they can be pu ...
Document
... Doppler shifts in the spectra of Mizar A and B, indicating that they are each binary stars. But they were too close to be directly imaged - until 2 May 1996, when the NPOI produced the first image of Mizar A. That image was the highest angular resolution image ever made in optical astronomy. Since t ...
... Doppler shifts in the spectra of Mizar A and B, indicating that they are each binary stars. But they were too close to be directly imaged - until 2 May 1996, when the NPOI produced the first image of Mizar A. That image was the highest angular resolution image ever made in optical astronomy. Since t ...
AST 207 Homework 7 Due 4 November 2011
... task is to think about what you learned. After doing a problem, identify the big ideas and the details. If you cannot identify what you learned immediately after doing a problem, you will certainly not be able to recall the ideas on a test. 1. In a few years, many of you will be teaching. A student ...
... task is to think about what you learned. After doing a problem, identify the big ideas and the details. If you cannot identify what you learned immediately after doing a problem, you will certainly not be able to recall the ideas on a test. 1. In a few years, many of you will be teaching. A student ...
Prep Homework Solutions for HW due 10/04/10
... the red giant in Algol used to be the more massive star, and it evolved off the Main Sequence before its companion, but then it lost significant mass through mass transfer to the companion, so the more massive star is the less massive star now. Note: a couple of you suggested that the paradox could ...
... the red giant in Algol used to be the more massive star, and it evolved off the Main Sequence before its companion, but then it lost significant mass through mass transfer to the companion, so the more massive star is the less massive star now. Note: a couple of you suggested that the paradox could ...
Constellations
... Asterism: Smaller groups of stars that form patterns within a constellation, from the Greek word aster, meaning star ...
... Asterism: Smaller groups of stars that form patterns within a constellation, from the Greek word aster, meaning star ...
Scientists classify stars by
... would look the same because the two lights are exactly the same. Their absolute magnitude is the same. Distance makes them look different. The same is true for stars. Two stars could be the same brightness but their distance from us makes their brightness different. ...
... would look the same because the two lights are exactly the same. Their absolute magnitude is the same. Distance makes them look different. The same is true for stars. Two stars could be the same brightness but their distance from us makes their brightness different. ...
Global Warming_Notes_for_Test_Review[1]
... 9. In most places around the world, there are four high tides and four low tides present each day. False – Two high tides and two low tides each day 10. A shooting star is often a star that passes through our atmosphere. False A shooting star is not a star. It is really a meteor. 11. The space betwe ...
... 9. In most places around the world, there are four high tides and four low tides present each day. False – Two high tides and two low tides each day 10. A shooting star is often a star that passes through our atmosphere. False A shooting star is not a star. It is really a meteor. 11. The space betwe ...
24exoplanets5s
... Would be able to detect the movement of a star in the sky as it is being pulled by its planets (astrometry) ...
... Would be able to detect the movement of a star in the sky as it is being pulled by its planets (astrometry) ...
JPL Small-Body Database Browser
... Proper Motion Proper motion was discovered by Edmund Halley. He compared the positions of bright stars that had been recorded by (Ptolemy). http://www.hwy.com.au/~sjquirk/images/film/barnard.html Barnard’s Star has the highest known proper motion of 10.3”/year. Even at that rate, Barnard’s Star wil ...
... Proper Motion Proper motion was discovered by Edmund Halley. He compared the positions of bright stars that had been recorded by (Ptolemy). http://www.hwy.com.au/~sjquirk/images/film/barnard.html Barnard’s Star has the highest known proper motion of 10.3”/year. Even at that rate, Barnard’s Star wil ...
2.7 - 2.9a
... of stars outlining an imaginary picture most have been identified since ancient times Constellations were once used to navigate by travelers because they appear to revolve around the North Star They ...
... of stars outlining an imaginary picture most have been identified since ancient times Constellations were once used to navigate by travelers because they appear to revolve around the North Star They ...
Astronomy practice questions for 3-6 test
... the G dwarf and from 100% to 85% in the case of the M dwarf. What is the radius of the planet relative to the G dwarf? Relative to the M dwarf? ...
... the G dwarf and from 100% to 85% in the case of the M dwarf. What is the radius of the planet relative to the G dwarf? Relative to the M dwarf? ...
Unit: Southern Europe
... GLE 0507.6.1: I can compare planets based on their known characteristics. This means that I can create a diagram, experiment or model communicating the major characteristics of each planet. I can also distinguish among the planets according to their appearance, location, composition, and apparent mo ...
... GLE 0507.6.1: I can compare planets based on their known characteristics. This means that I can create a diagram, experiment or model communicating the major characteristics of each planet. I can also distinguish among the planets according to their appearance, location, composition, and apparent mo ...
The Hertzsprung – Russell Diagram Star Data Table
... which type of star? (hint: red giant, main sequence, white dwarf) ...
... which type of star? (hint: red giant, main sequence, white dwarf) ...
Study Guide for the 4TH Astronomy Exam
... g. Describe the t-Tauri wind. h. Interpret the physical changes of a forming star on an HR diagram. i. Identify and define the ZAMS line on an HR diagram. j. Describe the relationship between OB associations and HII regions. 2. Main Sequence Stars a. List or identify the luminosity, mass, radius, te ...
... g. Describe the t-Tauri wind. h. Interpret the physical changes of a forming star on an HR diagram. i. Identify and define the ZAMS line on an HR diagram. j. Describe the relationship between OB associations and HII regions. 2. Main Sequence Stars a. List or identify the luminosity, mass, radius, te ...
Basic Observations of Stars
... Distances are Hard to Measure This took centuries of hard work following Galileo’s first use of an astronomical telescope, around 1600. Success came only in 1837 (as we will learn in the next few presentations). ...
... Distances are Hard to Measure This took centuries of hard work following Galileo’s first use of an astronomical telescope, around 1600. Success came only in 1837 (as we will learn in the next few presentations). ...
Solutions3
... First we find the distance from us to Mizar; use d = 1/p, get 23.8 pc. Now, we use θ = x/d (small angle formula) to find x (d=23.8 pc, θ=14.4”). To find it in parsecs, change θ into radians, θ = 7.02 × 10−5 radians, so x = 1.7 × 10−3 pc. In AU, we can just leave θ in arcseconds, so x = 343 AU. b) Fi ...
... First we find the distance from us to Mizar; use d = 1/p, get 23.8 pc. Now, we use θ = x/d (small angle formula) to find x (d=23.8 pc, θ=14.4”). To find it in parsecs, change θ into radians, θ = 7.02 × 10−5 radians, so x = 1.7 × 10−3 pc. In AU, we can just leave θ in arcseconds, so x = 343 AU. b) Fi ...
Take Something Like a Star
... It will not do to say of night, Since dark is what brings out your light. Some mystery becomes the proud. But to be wholly taciturn In your reserve is not allowed. Say something to us we can learn By heart and when alone repeat. Say something! And it says, “I burn.” But say with what degree of heat. ...
... It will not do to say of night, Since dark is what brings out your light. Some mystery becomes the proud. But to be wholly taciturn In your reserve is not allowed. Say something to us we can learn By heart and when alone repeat. Say something! And it says, “I burn.” But say with what degree of heat. ...
Our Universe
... “As Earth moves in its orbit around the sun, it changes position with respect to the stars; consequently, over time, people on Earth view the stars from slightly different positions. Astronomers calculate how these tiny variations in position correspond to the distance to a star.” ...
... “As Earth moves in its orbit around the sun, it changes position with respect to the stars; consequently, over time, people on Earth view the stars from slightly different positions. Astronomers calculate how these tiny variations in position correspond to the distance to a star.” ...
What tool do astronomers use to understand the evolution of stars?
... Luminosity, temperaure, radius Two stars are found to have the same luminosity. However, one star has twice the surface temperature of the other. From this information, what can you determine about their radii? A) The hotter star has half the radius of the cooler star. B) The cooler star has half t ...
... Luminosity, temperaure, radius Two stars are found to have the same luminosity. However, one star has twice the surface temperature of the other. From this information, what can you determine about their radii? A) The hotter star has half the radius of the cooler star. B) The cooler star has half t ...
3 rd stage of a star`s life = red giant
... Shells of gas thrown out by some stars near the end of their lives ...
... Shells of gas thrown out by some stars near the end of their lives ...
Star of Bethlehem
In Christian tradition, the Star of Bethlehem, also called the Christmas Star, revealed the birth of Jesus to the Biblical Magi, and later led them to Bethlehem. The star appears only in the nativity story of the Gospel of Matthew, where astrologers from the east are inspired by the star to travel to Jerusalem. There they meet King Herod of Judea, and ask where the king of the Jews had been born. Herod, following a verse from the Book of Micah interpreted as a prophecy, directs them to Bethlehem, to the south of Jerusalem. The star leads them to Jesus' home in the town, where they worship him and give him gifts. The wise men are then given a divine warning not to return to Herod so they return home by a different route.Many Christians see the star as a miraculous sign to mark the birth of the Christ (or messiah). Some theologians claimed that the star fulfilled a prophecy, known as the Star Prophecy. Astronomers have made several attempts to link the star to unusual astronomical events, such as a conjunction of Jupiter and Saturn, a comet or a supernova.Many modern scholars do not consider the story to be describing a historical event but a pious fiction created by the author of the Gospel of Matthew.The subject is a favorite at planetarium shows during the Christmas season, although the Biblical account describes Jesus with a broader Greek word, which can mean either ""infant"" or ""child"" (paidon), rather than the more specific word for infant (brephos), possibly implying that some time has passed since the birth. The visit is traditionally celebrated on Epiphany (January 6) in Western Christianity.