The fantastic journey of that ring on your finger: From
... The fantastic journey of that ring on your finger: From the Big Bang to your hand According to the prevailing Big Bang theory, the matter that made up the early universe largely consisted of hydrogen (the most basic element on the periodic table) and helium (the second gas on the scale). So, where d ...
... The fantastic journey of that ring on your finger: From the Big Bang to your hand According to the prevailing Big Bang theory, the matter that made up the early universe largely consisted of hydrogen (the most basic element on the periodic table) and helium (the second gas on the scale). So, where d ...
5. cosmic distance ladder ii: standard candles
... An object of known luminosity is called a standard candle. Most stars are not standard candles – their luminosities are not known and consequently their distances cannot be easily calculated. However, some special types of variable and exploding stars do have known, standard luminosities. Consequen ...
... An object of known luminosity is called a standard candle. Most stars are not standard candles – their luminosities are not known and consequently their distances cannot be easily calculated. However, some special types of variable and exploding stars do have known, standard luminosities. Consequen ...
supplemental educational materials PDF
... they are visible in the northern sky all year long. These include: Ursa Major, the Great Bear; Ursa Minor, the Small Bear; Draco, the Dragon; Cassiopeia, the Queen of Ethiopia; and Cepheus, the King of Ethiopia. • Students may incorrectly identify the Big Dipper or the Pleiades as constellations, bu ...
... they are visible in the northern sky all year long. These include: Ursa Major, the Great Bear; Ursa Minor, the Small Bear; Draco, the Dragon; Cassiopeia, the Queen of Ethiopia; and Cepheus, the King of Ethiopia. • Students may incorrectly identify the Big Dipper or the Pleiades as constellations, bu ...
Chapter 10 Measuring the Stars: Giants, Dwarfs, and the Main
... * Some stars are supergiants and are also located near the top right (_______________) * White dwarfs are hot, faint, small stars near the bottom of the diagram • Some white dwarfs are Earth sized * Bright and near stars plotted on diagram Extending the Cosmic Distance Scale * Spectroscopic Parallax ...
... * Some stars are supergiants and are also located near the top right (_______________) * White dwarfs are hot, faint, small stars near the bottom of the diagram • Some white dwarfs are Earth sized * Bright and near stars plotted on diagram Extending the Cosmic Distance Scale * Spectroscopic Parallax ...
Investigate Stars and Galaxies - American Museum of Natural History
... Lower Level (40 minutes) Using their student worksheets, have students visit the following two locations to collect evidence about stars. They can explore individually, in pairs, or in small groups. ...
... Lower Level (40 minutes) Using their student worksheets, have students visit the following two locations to collect evidence about stars. They can explore individually, in pairs, or in small groups. ...
Luminosity
... These two stars have about the same luminosity— which one appears brighter? A. Alpha Centauri B. The Sun ...
... These two stars have about the same luminosity— which one appears brighter? A. Alpha Centauri B. The Sun ...
Learning Objectives
... An object of known luminosity is called a standard candle. Most stars are not standard candles – their luminosities are not known and consequently their distances cannot be easily calculated. However, some special types of variable and exploding stars do have known, standard luminosities. Consequen ...
... An object of known luminosity is called a standard candle. Most stars are not standard candles – their luminosities are not known and consequently their distances cannot be easily calculated. However, some special types of variable and exploding stars do have known, standard luminosities. Consequen ...
slides
... Q: Which is larger? A. K-type main sequence star B. K-type giant C. they are about the same ...
... Q: Which is larger? A. K-type main sequence star B. K-type giant C. they are about the same ...
The Hertzsprung-Russell diagram and the nature of stars
... • Physical argument 1: what holds stars up? • Physical argument 2: what powers the stars (where do they get their energy supply?) ...
... • Physical argument 1: what holds stars up? • Physical argument 2: what powers the stars (where do they get their energy supply?) ...
David`s Mapping the Heavens[1]
... Complete the following table. In each column outline what theory each astronomer came up with. Shapley ...
... Complete the following table. In each column outline what theory each astronomer came up with. Shapley ...
The Stars and the Solar System
... patterns, and planets. a. Recognize the physical attributes of stars in the night sky such as number, size, color, and patterns. ...
... patterns, and planets. a. Recognize the physical attributes of stars in the night sky such as number, size, color, and patterns. ...
The Stars and the Solar System
... patterns, and planets. a. Recognize the physical attributes of stars in the night sky such as number, size, color, and patterns. ...
... patterns, and planets. a. Recognize the physical attributes of stars in the night sky such as number, size, color, and patterns. ...
Star Types - University of Massachusetts Amherst
... the deaths of high mass stars (supernovae). We were all once fuel for a stellar furnace. Parts of us were formed in a supernova. ...
... the deaths of high mass stars (supernovae). We were all once fuel for a stellar furnace. Parts of us were formed in a supernova. ...
Participant Handout - Math Machines Home
... discovered that temperature (measure in kelvin) is inversely proportional to the wavelength of a star’s peak emission as described by the equation: λmax T= 3,000,000 nm K The actual brightness (luminosity) of a star is determined by the star’s size and temperature. In addition to having a more blui ...
... discovered that temperature (measure in kelvin) is inversely proportional to the wavelength of a star’s peak emission as described by the equation: λmax T= 3,000,000 nm K The actual brightness (luminosity) of a star is determined by the star’s size and temperature. In addition to having a more blui ...
Eksamination in FY2450 Astrophysics Wednesday June 8
... spectral classes, OBAFGKM, is a reversed temperature axis. With increasing temperature, when we go from right to left in the plot, a given spectral line first appears when the temperature becomes high enough that photons get enough energy to excite the atoms (or molecules). The line is strongest whe ...
... spectral classes, OBAFGKM, is a reversed temperature axis. With increasing temperature, when we go from right to left in the plot, a given spectral line first appears when the temperature becomes high enough that photons get enough energy to excite the atoms (or molecules). The line is strongest whe ...
CCD BVRI and 2MASS Photometry of the Poorly Studied Open
... NGC 6631. It is observed from the 1.88 m Telescope of Kottamia Observatory in Egypt. About 3300 stars have been observed in an area of ∼ 10′ × 10′ around the cluster center. The main photometric parameters have been estimated and compared with the results that determined for the cluster using JHKs 2 ...
... NGC 6631. It is observed from the 1.88 m Telescope of Kottamia Observatory in Egypt. About 3300 stars have been observed in an area of ∼ 10′ × 10′ around the cluster center. The main photometric parameters have been estimated and compared with the results that determined for the cluster using JHKs 2 ...
Combining Practices with Core Ideas in the NGSS
... To illustrate how the distances to the nearest stars are measured, I could have the students use a graphical method to measure how far it is to a distant object on the playground by measuring angles to the object from two ends of a baseline (which connects with Common Core State Standards for 5th gr ...
... To illustrate how the distances to the nearest stars are measured, I could have the students use a graphical method to measure how far it is to a distant object on the playground by measuring angles to the object from two ends of a baseline (which connects with Common Core State Standards for 5th gr ...
Star Powerpoint notes
... miles) away. It takes light about 4 years to reach the Earth from there. How luminous is the Sun compared with other stars? The most luminous stars are about a million times brighter and the least luminous stars are about a hundred thousand times dimmer than the Sun. ...
... miles) away. It takes light about 4 years to reach the Earth from there. How luminous is the Sun compared with other stars? The most luminous stars are about a million times brighter and the least luminous stars are about a hundred thousand times dimmer than the Sun. ...
UNIT VIII/B: THE EARTH IN SPACE – STARS AND GALAXIES
... a. A light-year is a unit of distance (NOT TIME!!!). It is the distance that light can travel in one year. b. Light moves at a velocity of about 300,000 km each second (in a vacuum). So in one year, it can travel about 10 trillion km. More precisely, one light-year is equal to 9,460,500,000,000 kilo ...
... a. A light-year is a unit of distance (NOT TIME!!!). It is the distance that light can travel in one year. b. Light moves at a velocity of about 300,000 km each second (in a vacuum). So in one year, it can travel about 10 trillion km. More precisely, one light-year is equal to 9,460,500,000,000 kilo ...
Distance - courses.psu.edu
... 6. A certain star is known to be equal in luminosity to the Sun, but its measured flux is only 1/10,000 (one ten-thousandth) the Sun's flux. What would be the distance to this star, in AU? 7. Two stars, A and B, are known to be equal in luminosity, but A appears 16 times brighter (as viewed from Ear ...
... 6. A certain star is known to be equal in luminosity to the Sun, but its measured flux is only 1/10,000 (one ten-thousandth) the Sun's flux. What would be the distance to this star, in AU? 7. Two stars, A and B, are known to be equal in luminosity, but A appears 16 times brighter (as viewed from Ear ...
Astronomy Final Study Guide – Name: **This will be the biggest test
... 22. How does the atmosphere protect us from dangerous forms of radiation? Which forms does it protect us from? Be able to draw a diagram explaining how this happens. ...
... 22. How does the atmosphere protect us from dangerous forms of radiation? Which forms does it protect us from? Be able to draw a diagram explaining how this happens. ...
ppt
... • An open cluster is a group of up to a few thousand stars that were formed from the same giant molecular cloud, and are still gravitationally bound to each other • Open clusters are found only in spiral and irregular galaxies, in which active star formation is occurring. • The Pleiades is an open c ...
... • An open cluster is a group of up to a few thousand stars that were formed from the same giant molecular cloud, and are still gravitationally bound to each other • Open clusters are found only in spiral and irregular galaxies, in which active star formation is occurring. • The Pleiades is an open c ...
Perseus (constellation)
Perseus, named after the Greek mythological hero Perseus, is a constellation in the northern sky. It was one of 48 listed by the 2nd-century astronomer Ptolemy and among the 88 modern constellations defined by the International Astronomical Union (IAU). It is located in the northern celestial hemisphere near several other constellations named after legends surrounding Perseus, including Andromeda to the west and Cassiopeia to the north. Perseus is also bordered by Aries and Taurus to the south, Auriga to the east, Camelopardalis to the north, and Triangulum to the west.The galactic plane of the Milky Way passes through Perseus but is mostly obscured by molecular clouds. The constellation's brightest star is the yellow-white supergiant Alpha Persei (also called Mirfak), which shines at magnitude 1.79. It and many of the surrounding stars are members of an open cluster known as the Alpha Persei Cluster. The best-known star, however, is Algol (Beta Persei), linked with ominous legends because of its variability, which is noticeable to the naked eye. Rather than being an intrinsically variable star, it is an eclipsing binary. Other notable star systems in Perseus include X Persei, a binary system containing a neutron star, and GK Persei, a nova that peaked at magnitude 0.2 in 1901. The Double Cluster, comprising two open clusters quite near each other in the sky, was known to the ancient Chinese. The constellation gives its name to the Perseus Cluster (Abell 426), a massive galaxy cluster located 250 million light-years from Earth. It hosts the radiant of the annual Perseids meteor shower—one of the most prominent meteor showers in the sky.