
Science 8
... 13. The hottest stars are what color? _________________________________ 14. A red star is hotter / cooler than a yellow star. 15. A white star is hotter / cooler than an orange star. 16. Our sun is a ____________(color) star and is approximately __________(temperature) ...
... 13. The hottest stars are what color? _________________________________ 14. A red star is hotter / cooler than a yellow star. 15. A white star is hotter / cooler than an orange star. 16. Our sun is a ____________(color) star and is approximately __________(temperature) ...
Almach or Alberio
... daytime star. The dimmer blue star (known as Almach B,C, and D) is also actually a triple system of three white dwarf stars . The white dwarf stars together orbit the gold primary star at a distance of about 600 AU (600 times the Sun-Earth distance). Although the golden primary is 9.6 arc seconds on ...
... daytime star. The dimmer blue star (known as Almach B,C, and D) is also actually a triple system of three white dwarf stars . The white dwarf stars together orbit the gold primary star at a distance of about 600 AU (600 times the Sun-Earth distance). Although the golden primary is 9.6 arc seconds on ...
OUSNMAR05 - The Open University
... orientation of the map may differ from that of the observed image of the Moon depending on the type of telescope used. If you find the Moon too bright use a filter to reduce the glare. At times features along different parts of the limb are better presented due the effect of libration – an apparent ...
... orientation of the map may differ from that of the observed image of the Moon depending on the type of telescope used. If you find the Moon too bright use a filter to reduce the glare. At times features along different parts of the limb are better presented due the effect of libration – an apparent ...
Winter constellations
... Taurus, the Bull, with another prominent red star, Aldebaran, making up the eye of the Bull. The Taurus constellation looks particularly brilliant with binoculars, glittering with young blue stars. Aldebaran is a red supergiant star and is about five times the mass of the sun. The name means ‘follow ...
... Taurus, the Bull, with another prominent red star, Aldebaran, making up the eye of the Bull. The Taurus constellation looks particularly brilliant with binoculars, glittering with young blue stars. Aldebaran is a red supergiant star and is about five times the mass of the sun. The name means ‘follow ...
Chapter 27 Stars and Galaxies
... Absolute Magnitude Brightness from 32.6 ly Ex: If the sun was 32.6 ly away, it would be a fifth magnitude star. Its absolute magnitude = +5 Most stars are between a -5 and +15 ...
... Absolute Magnitude Brightness from 32.6 ly Ex: If the sun was 32.6 ly away, it would be a fifth magnitude star. Its absolute magnitude = +5 Most stars are between a -5 and +15 ...
new_qwk11
... the Special Theory of Relativity B. The General Theory of Relativity was designed to explain situations where the speeds of objects are close to the speed of light C. The Special Theory of Relativity states that a moving ruler is measured to be longer than its twin ruler at rest D. The mass or inert ...
... the Special Theory of Relativity B. The General Theory of Relativity was designed to explain situations where the speeds of objects are close to the speed of light C. The Special Theory of Relativity states that a moving ruler is measured to be longer than its twin ruler at rest D. The mass or inert ...
The Lifecycle of Stars
... to document the stages of a star’s lifecycle. Using the paper I provide, you will have to design and ...
... to document the stages of a star’s lifecycle. Using the paper I provide, you will have to design and ...
February - Bristol Astronomical Society
... This famous cluster has been known since prehistoric times. The ancient Greeks saw this "nebula" as the manger (Phatne) associated with two asses who eat from it, Asellus Borealis, the Northern Ass (Gamma Cnc) and Asellus Australis, the Southern Ass (Delta Cnc). Erathosthenes reported that these wer ...
... This famous cluster has been known since prehistoric times. The ancient Greeks saw this "nebula" as the manger (Phatne) associated with two asses who eat from it, Asellus Borealis, the Northern Ass (Gamma Cnc) and Asellus Australis, the Southern Ass (Delta Cnc). Erathosthenes reported that these wer ...
Star Study Guide Chapter 21 Test
... shows the relationship between absolute brightness and surface temperature of a star ...
... shows the relationship between absolute brightness and surface temperature of a star ...
a geolocation. Obtain the information related to certain star.
... Alvaro Graves, James Michaelis, Joshua Shinavier and Giovanni Thenstead Rensselaer Polytechnic Institute Troy, NY, USA ...
... Alvaro Graves, James Michaelis, Joshua Shinavier and Giovanni Thenstead Rensselaer Polytechnic Institute Troy, NY, USA ...
Homework Problems for Quiz 1 – AY 5 – Spring 2013
... b) what are the relative brightnesses of the two stars? ...
... b) what are the relative brightnesses of the two stars? ...
Discussion Activity #10
... A. Both stars have the same luminosity, but the apparent brightness of the closer star is four times as great as that of the more distant star. B. Both stars have the same apparent brightness, but the luminosity of the closer star is four times as great as that of the more distant star. C. Both star ...
... A. Both stars have the same luminosity, but the apparent brightness of the closer star is four times as great as that of the more distant star. B. Both stars have the same apparent brightness, but the luminosity of the closer star is four times as great as that of the more distant star. C. Both star ...
Astronomy Objectives
... The Hubble Law; state it and describe the evidence that supports it Big Bang Theory: be able to explain how the universe was formed according to this theory; know the particles formed at each step, but not specific times or temperatures ...
... The Hubble Law; state it and describe the evidence that supports it Big Bang Theory: be able to explain how the universe was formed according to this theory; know the particles formed at each step, but not specific times or temperatures ...
Magnitude Scale
... • Measure of the brightness of a star if observed from 10 parsecs away (equivalent of luminosity) • Denoted by M or MV • Absolute magnitude and apparent magnitude are the same at a distance of 10 parsecs. ...
... • Measure of the brightness of a star if observed from 10 parsecs away (equivalent of luminosity) • Denoted by M or MV • Absolute magnitude and apparent magnitude are the same at a distance of 10 parsecs. ...
1” “Sky-Notes” of the Open University Astronomy Club. October 2005
... month occur on the 17th and 20th. Delta () Cephei. +3.5 to +4.4, period 5.37 days. The prototype for the Cepheid class of variable stars. Their period-luminosity relationship has lead them to being used as “standard candles” in measuring distances to nearby galaxies. Maximum brightness occurs on 6t ...
... month occur on the 17th and 20th. Delta () Cephei. +3.5 to +4.4, period 5.37 days. The prototype for the Cepheid class of variable stars. Their period-luminosity relationship has lead them to being used as “standard candles” in measuring distances to nearby galaxies. Maximum brightness occurs on 6t ...
Day-6
... An individual star follows an evolutionary track on the H-R diagram. This is the path of the temperature and luminosity with time. Protostars get less luminous and hotter. The star first appears as a T Tauri star. The star moves on the Hayashi track and arrives on the main sequence. Sinc ...
... An individual star follows an evolutionary track on the H-R diagram. This is the path of the temperature and luminosity with time. Protostars get less luminous and hotter. The star first appears as a T Tauri star. The star moves on the Hayashi track and arrives on the main sequence. Sinc ...
The Stars
... 4. describe the process by which the sun generates energy. 5. describe the internal structure of the sun. 6. define the solar wind, and indicate its effects on the planets. 7. describe three major types of stars (main sequence, supergiants, white dwarfs) in a stellar cycle. 8. interpret a Hertzsprun ...
... 4. describe the process by which the sun generates energy. 5. describe the internal structure of the sun. 6. define the solar wind, and indicate its effects on the planets. 7. describe three major types of stars (main sequence, supergiants, white dwarfs) in a stellar cycle. 8. interpret a Hertzsprun ...
E3 STELLAR DISTANCES E4 COSMOLOGY
... A main sequence star emits most of its energy at λ = 2.4 x 10-7 m. Its apparent brightness is measure at 4.3 x 10-9 W m-2. How far away is the star? [28 pc] ...
... A main sequence star emits most of its energy at λ = 2.4 x 10-7 m. Its apparent brightness is measure at 4.3 x 10-9 W m-2. How far away is the star? [28 pc] ...
The HR Diagram and Stars Worksheet
... a. Page 622 – Add the Spectral Class below the temperatures. b. Page 626 – Use colored pencils to add and label the band that represents Main Sequence stars. c. Page 626 – Use colored pencils to label the following areas: Blue Giants, Red Super Giants, Red Giants, Red Dwarfs, White Dwarfs d. Page 62 ...
... a. Page 622 – Add the Spectral Class below the temperatures. b. Page 626 – Use colored pencils to add and label the band that represents Main Sequence stars. c. Page 626 – Use colored pencils to label the following areas: Blue Giants, Red Super Giants, Red Giants, Red Dwarfs, White Dwarfs d. Page 62 ...
Extension worksheet – Topic 6 - Cambridge Resources for the IB
... Two main sequence stars have masses of 2 M e and 10 M e . Compare the evolutionary paths of these two stars with reference to a ...
... Two main sequence stars have masses of 2 M e and 10 M e . Compare the evolutionary paths of these two stars with reference to a ...
F03HW09
... Why are earth-based parallax measurements limited to the nearest stars? Parallax measurements are limited because we measure the motion of a star due to the motion of Earth around the sun. Earth’s orbit is so small compared to the distance to stars that even the nearest stars show very small apparen ...
... Why are earth-based parallax measurements limited to the nearest stars? Parallax measurements are limited because we measure the motion of a star due to the motion of Earth around the sun. Earth’s orbit is so small compared to the distance to stars that even the nearest stars show very small apparen ...
Stars and Galaxies - Earth Science: Astronomy
... disrupt radio signals b. Near Earth’s polar areas solar wind material can create light called an aurora ...
... disrupt radio signals b. Near Earth’s polar areas solar wind material can create light called an aurora ...
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.