Slide 1
... processes within the body of the star itself. Stars typically range in mass between 0.08 and 100 solar masses. A Hertzprung-Russell diagram is a very useful illustration of the relationship between various key stellar properties, namely the luminosity and the effective temperature (related to both s ...
... processes within the body of the star itself. Stars typically range in mass between 0.08 and 100 solar masses. A Hertzprung-Russell diagram is a very useful illustration of the relationship between various key stellar properties, namely the luminosity and the effective temperature (related to both s ...
The Life of a Star - Department of Physics and Astronomy
... Young star clusters give insight into star formation and evolution • Newborn stars may form an open or galactic cluster • Stars are held together in such a cluster by gravity • Occasionally a star moving more rapidly than average will escape, or leave the cluster • A stellar association is a group ...
... Young star clusters give insight into star formation and evolution • Newborn stars may form an open or galactic cluster • Stars are held together in such a cluster by gravity • Occasionally a star moving more rapidly than average will escape, or leave the cluster • A stellar association is a group ...
ASTR-1020: Astronomy II Course Lecture Notes Section III
... Example III–7. We measure the trigonometric parallax of a visual binary star as 0.20 arcsec and measure an angular separation between the pair of stars in this binary as 5 arcsec. Over a few years of observations, we determine the orbital period of this pair to be 30 years. What is the combined mass ...
... Example III–7. We measure the trigonometric parallax of a visual binary star as 0.20 arcsec and measure an angular separation between the pair of stars in this binary as 5 arcsec. Over a few years of observations, we determine the orbital period of this pair to be 30 years. What is the combined mass ...
- Stevenson High School
... stars are circumpolar (perpetually in the sky, even over a 24 hours’ period). Which one of the constellations below besides Little Dipper contains stars that are circumpolar for our mid-northern hemisphere Star Wheel observer? a) Betelgeuse b) Sagittarius c) Cepheus d) Taurus 22. The daily motion of ...
... stars are circumpolar (perpetually in the sky, even over a 24 hours’ period). Which one of the constellations below besides Little Dipper contains stars that are circumpolar for our mid-northern hemisphere Star Wheel observer? a) Betelgeuse b) Sagittarius c) Cepheus d) Taurus 22. The daily motion of ...
Astronomy Exam #2 for the 10
... The hot main sequence stars appear to be mostly B and A spectral type with an absolute magnitude between +2 and -5. This range in absolute magnitudes corresponds to a range in luminosity of between 16 and 10,000 solar luminosities. These stars will have a short main sequence lifetime compared to the ...
... The hot main sequence stars appear to be mostly B and A spectral type with an absolute magnitude between +2 and -5. This range in absolute magnitudes corresponds to a range in luminosity of between 16 and 10,000 solar luminosities. These stars will have a short main sequence lifetime compared to the ...
Indoor lab #1: The Hertzsprung-Russel Diagram and Selection Effects
... a) the average distance of all the stars in your table: b) the number of and average distance of the red giant stars (stars of type 1) c) the number of and average distance of the bluer main sequence stars (stars of type 2) d) the number of and average distance of the redder main sequence stars (sta ...
... a) the average distance of all the stars in your table: b) the number of and average distance of the red giant stars (stars of type 1) c) the number of and average distance of the bluer main sequence stars (stars of type 2) d) the number of and average distance of the redder main sequence stars (sta ...
Starry Night¨ Times - October 2008
... area 20 lightyears in width. Bright enough to be sometimes visible to the naked eye (Aristotle is said to have noticed it around 325 B.C.) M41 is a good target for binos or low magnification in your scope. M46 and M47 are two open clusters just over 1° apart, making comparison very easy. Both are ab ...
... area 20 lightyears in width. Bright enough to be sometimes visible to the naked eye (Aristotle is said to have noticed it around 325 B.C.) M41 is a good target for binos or low magnification in your scope. M46 and M47 are two open clusters just over 1° apart, making comparison very easy. Both are ab ...
Life Cycle of a Star
... Within the range of this spectrum, there are yellow or orange stars (like our sun which is a G star) and white stars. White stars contain mostly green emissions but since green is in the middle of the color spectrum, they blend together and the color we see is white. Sadly there are no green stars. ...
... Within the range of this spectrum, there are yellow or orange stars (like our sun which is a G star) and white stars. White stars contain mostly green emissions but since green is in the middle of the color spectrum, they blend together and the color we see is white. Sadly there are no green stars. ...
HR Diagram and Life of a star
... Much Brighter than the main Sequence stars of the same temp This means that they are very large and can range in size from 100-1000 times the size of the sun GIANTS- large bright stars a bit smaller and fainter than Super giants Super giants in the Red temp range tend to be in their last stages of l ...
... Much Brighter than the main Sequence stars of the same temp This means that they are very large and can range in size from 100-1000 times the size of the sun GIANTS- large bright stars a bit smaller and fainter than Super giants Super giants in the Red temp range tend to be in their last stages of l ...
Universe 8e Lecture Chapter 17 Nature of Stars
... sequence star or a white dwarf. These define the luminosity classes shown on the left occupying distinct regions on the HR diagram. ...
... sequence star or a white dwarf. These define the luminosity classes shown on the left occupying distinct regions on the HR diagram. ...
Lives of Stars - Madison County Schools
... Our solar system formed from this type of scenario. All of the material for everything in this solar system came from a supernova that exploded in this area of the Milky Way. ...
... Our solar system formed from this type of scenario. All of the material for everything in this solar system came from a supernova that exploded in this area of the Milky Way. ...
Measuring Stars
... Star A and star B are equally bright, but star A is farther away. Which one is actually more luminous? A) Star A B) Star B C) They are equally luminous D) There is insufficient information ...
... Star A and star B are equally bright, but star A is farther away. Which one is actually more luminous? A) Star A B) Star B C) They are equally luminous D) There is insufficient information ...
Apparent Magnitude
... (hot and bright) to the lower-right (cooler and less bright), called the main sequence. In the lower-left is where white dwarfs are found, and above the main sequence are the subgiants, giants and supergiants. The Sun is found on the main sequence at luminosity 1 and temperature 5780K (spectral type ...
... (hot and bright) to the lower-right (cooler and less bright), called the main sequence. In the lower-left is where white dwarfs are found, and above the main sequence are the subgiants, giants and supergiants. The Sun is found on the main sequence at luminosity 1 and temperature 5780K (spectral type ...
CONSTELLATIONS
... As you have seen, the dashed line on the planisphere marks the ecliptic. As our Earth moves around in its orbit, the Sun, the Moon, and the planets also appear along this line. The ecliptic therefore represents the plane of the solar system. Of the nine planets, five are easily visible without a tel ...
... As you have seen, the dashed line on the planisphere marks the ecliptic. As our Earth moves around in its orbit, the Sun, the Moon, and the planets also appear along this line. The ecliptic therefore represents the plane of the solar system. Of the nine planets, five are easily visible without a tel ...
The Celestial Sphere - Department of Physics and Astronomy
... However some stars show small motions, these are due again to the motion of the Earth. An object that moves 1 second of arc in the sky (1/3600 of a degree) as the Earth moves 1 AU in its orbit in 1 ...
... However some stars show small motions, these are due again to the motion of the Earth. An object that moves 1 second of arc in the sky (1/3600 of a degree) as the Earth moves 1 AU in its orbit in 1 ...
Lecture 19 Brightness Units
... are all due to absorption by atoms starting from the second energy state. – The only way an atom gets into this state is by being hit by a neighbor, and the neighbors at these temperatures are not moving fast enough. Balmer lines are weak. Mar 3, 2006 ...
... are all due to absorption by atoms starting from the second energy state. – The only way an atom gets into this state is by being hit by a neighbor, and the neighbors at these temperatures are not moving fast enough. Balmer lines are weak. Mar 3, 2006 ...
HERE
... The pulsations can be regular or irregular, ranging from more than a year to only a few hours between pulsations. The change in size by about 15% of their radius. For more info in Pulsating Variable Stars, you can visit: http://faculty.rmwc.edu/tmichalik/pulsvar.htm ...
... The pulsations can be regular or irregular, ranging from more than a year to only a few hours between pulsations. The change in size by about 15% of their radius. For more info in Pulsating Variable Stars, you can visit: http://faculty.rmwc.edu/tmichalik/pulsvar.htm ...
1. Stellar Evolution – Notes Astronomers classify stars according to
... star can be described in two different ways: apparent brightness and absolute brightness. A star’s apparent brightness is its brightness as seen from Earth. Astronomers can measure apparent brightness fairly easily using electronic devices. A star’s absolute brightness is the brightness the star wou ...
... star can be described in two different ways: apparent brightness and absolute brightness. A star’s apparent brightness is its brightness as seen from Earth. Astronomers can measure apparent brightness fairly easily using electronic devices. A star’s absolute brightness is the brightness the star wou ...
HR-Diagram
... FORMATION- Space contains gas and dust and stars are formed in nurseries called Nebulas or a contracting cloud of dust and gas Some Nebulas glow while others are dark Stars are created from Gravity pulling the nebula together and making a dense ball of gas PROTOSTAR- enough gas and dust to form a st ...
... FORMATION- Space contains gas and dust and stars are formed in nurseries called Nebulas or a contracting cloud of dust and gas Some Nebulas glow while others are dark Stars are created from Gravity pulling the nebula together and making a dense ball of gas PROTOSTAR- enough gas and dust to form a st ...
Star Life Cycle Powerpoin
... • Outer shell expands from 1 to at least 40 million miles across. ( 10 to 100 times larger than the Sun) ...
... • Outer shell expands from 1 to at least 40 million miles across. ( 10 to 100 times larger than the Sun) ...
stars_2nd_edit
... years for massive stars to billions for smaller stars. Our Sun, which is of average mass, is predicted to live for about 10 billion years. By knowing the distance, mass, magnitude, and chemical composition of a star, we can determine approximately how old it is, when it was born, and when it will di ...
... years for massive stars to billions for smaller stars. Our Sun, which is of average mass, is predicted to live for about 10 billion years. By knowing the distance, mass, magnitude, and chemical composition of a star, we can determine approximately how old it is, when it was born, and when it will di ...
Stars
... Life span of a star depends on its size. – Very large, massive stars burn their fuel much faster than smaller stars – Main sequence may last only a few hundred thousand years – Smaller stars will live on for billions of years because they burn their fuel much more slowly ...
... Life span of a star depends on its size. – Very large, massive stars burn their fuel much faster than smaller stars – Main sequence may last only a few hundred thousand years – Smaller stars will live on for billions of years because they burn their fuel much more slowly ...
chapter10
... Low luminosity; high temperature => White dwarfs are found in the lower center/left of the H-R diagram. ...
... Low luminosity; high temperature => White dwarfs are found in the lower center/left of the H-R diagram. ...
Canis Minor
Canis Minor /ˌkeɪnɨs ˈmaɪnər/ is a small constellation in the northern celestial hemisphere. In the second century, it was included as an asterism, or pattern, of two stars in Ptolemy's 48 constellations, and it is counted among the 88 modern constellations. Its name is Latin for ""lesser dog"", in contrast to Canis Major, the ""greater dog""; both figures are commonly represented as following the constellation of Orion the hunter.Canis Minor contains only two stars brighter than the fourth magnitude, Procyon (Alpha Canis Minoris), with a magnitude of 0.34, and Gomeisa (Beta Canis Minoris), with a magnitude of 2.9. The constellation's dimmer stars were noted by Johann Bayer, who named eight stars including Alpha and Beta, and John Flamsteed, who numbered fourteen. Procyon is the seventh-brightest star in the night sky, as well as one of the closest. A yellow-white main sequence star, it has a white dwarf companion. Gomeisa is a blue-white main sequence star. Luyten's Star is a ninth-magnitude red dwarf and the Solar System's next closest stellar neighbour in the constellation after Procyon. The fourth-magnitude HD 66141, which has evolved into an orange giant towards the end of its life cycle, was discovered to have a planet in 2012. There are two faint deep sky objects within the constellation's borders. The 11 Canis-Minorids are a meteor shower that can be seen in early December.