April 2005
... • Can be viewed indirectly by observing the back-and-forth Doppler shifts of their ...
... • Can be viewed indirectly by observing the back-and-forth Doppler shifts of their ...
Homework 2 (Due Sept 18, 2014)
... with an orbital period of 63 days. What is the planet’s orbital distance?! d. Pluto’s moon Charon orbits Pluto every 6.4 days with a semimajor axis of 19,700 km. Calculate the combined mass of Pluto and Charon.! e. Calculate the orbital period of a spacecraft in an orbit 300 kilometers above Earth’s ...
... with an orbital period of 63 days. What is the planet’s orbital distance?! d. Pluto’s moon Charon orbits Pluto every 6.4 days with a semimajor axis of 19,700 km. Calculate the combined mass of Pluto and Charon.! e. Calculate the orbital period of a spacecraft in an orbit 300 kilometers above Earth’s ...
about Stars
... • Astronomers quantify the “color” of a star by using the difference in brightness between the brightness in the B and V spectral regions • The B-V color is related to the slope of the ...
... • Astronomers quantify the “color” of a star by using the difference in brightness between the brightness in the B and V spectral regions • The B-V color is related to the slope of the ...
Astronomy
... The Big Dipper points to the North Star. People at the North Pole can see the North Star. People in Australia can see the Big Dipper. The Big Dipper is out during the Daytime. The North Star is out during the Daytime.* Unlike the others (which are true), People in Australia cannot see the Big Dipper ...
... The Big Dipper points to the North Star. People at the North Pole can see the North Star. People in Australia can see the Big Dipper. The Big Dipper is out during the Daytime. The North Star is out during the Daytime.* Unlike the others (which are true), People in Australia cannot see the Big Dipper ...
Determining the Sizes & Distances of Stars Using the H
... ● Giants: Giants are stars that have begun to evolve after finishing their time as a main sequence star. Their cores have filled with helium. There is not enough hydrogen left in the core so burning occurs in a shell surrounding the core, where more helium resides. In the process, the star grows in ...
... ● Giants: Giants are stars that have begun to evolve after finishing their time as a main sequence star. Their cores have filled with helium. There is not enough hydrogen left in the core so burning occurs in a shell surrounding the core, where more helium resides. In the process, the star grows in ...
The Spatially-Resolved Scaling Law of Star Formation
... know that they exist? • The star HD 226868 is an excellent example. It is a B supergiant. • The spectral lines in the star clearly show that it is in a binary system with a period of 5.6 days, however, we see no companion star. ...
... know that they exist? • The star HD 226868 is an excellent example. It is a B supergiant. • The spectral lines in the star clearly show that it is in a binary system with a period of 5.6 days, however, we see no companion star. ...
Study Guide for 1ST Astronomy Exam
... speed of travel, t=d/v, Using a proportion, calculate how big an object would be given the model size of another object. e.g. “If the Earth were the size of a softball (diameter = 8 cm, how big would the Milky Way galaxy be?”, Unit 3: Astronomical Numbers Convert between cm, m and km, Work in ...
... speed of travel, t=d/v, Using a proportion, calculate how big an object would be given the model size of another object. e.g. “If the Earth were the size of a softball (diameter = 8 cm, how big would the Milky Way galaxy be?”, Unit 3: Astronomical Numbers Convert between cm, m and km, Work in ...
Analysis of Two Pulsating X-ray Sources
... The SS Cygni light curve above was observed in the optical part of the spectrum and displays the dynamics among the accretion disk – the material in the disk that was accreted from its companion star – and the surface of the white dwarf. The white dwarf itself is the stellar core of a Sun-sized star ...
... The SS Cygni light curve above was observed in the optical part of the spectrum and displays the dynamics among the accretion disk – the material in the disk that was accreted from its companion star – and the surface of the white dwarf. The white dwarf itself is the stellar core of a Sun-sized star ...
Grand Tour Worksheet - School District of La Crosse
... 12. Distances in the solar system are measured in __________ ___________, and this is how far? 13. How far is the sun from Saturn in A.U.’s 14. Pluto is how many A.U.’s? ...
... 12. Distances in the solar system are measured in __________ ___________, and this is how far? 13. How far is the sun from Saturn in A.U.’s 14. Pluto is how many A.U.’s? ...
Stefan-Boltzmann`s law Wien`s law
... maximum wavelength corresponding to a black body spectrum of an extremely cold object of temperature of 2.7 K. Cosmological background radiation / Cosmic microwave background radiation (CMB) is microwave radiation - left over from the Big Bang that fills the universe roughly uniformly in all directi ...
... maximum wavelength corresponding to a black body spectrum of an extremely cold object of temperature of 2.7 K. Cosmological background radiation / Cosmic microwave background radiation (CMB) is microwave radiation - left over from the Big Bang that fills the universe roughly uniformly in all directi ...
Pluto`s Bald Cousin
... until it was downgraded to a dwarf planet like Makemake. Dwarf planets are basically too small to be labelled as planets, but they still are spherical objects – like planets – and bigger than asteroids. We know very little about our closer dwarf planets, and knew practically nothing about Makemake. ...
... until it was downgraded to a dwarf planet like Makemake. Dwarf planets are basically too small to be labelled as planets, but they still are spherical objects – like planets – and bigger than asteroids. We know very little about our closer dwarf planets, and knew practically nothing about Makemake. ...
Galactic Structure
... field halo must have been accreted/disrupted prior to self-enrichment by Type Ia supernovae And also formed stars only a long time ago, so if similar to surviving satellites and would have extended SFH, need to have been accreted a long time (~10Gyr) ago ...
... field halo must have been accreted/disrupted prior to self-enrichment by Type Ia supernovae And also formed stars only a long time ago, so if similar to surviving satellites and would have extended SFH, need to have been accreted a long time (~10Gyr) ago ...
Earth Dimensions
... survive and our weather. The other three layers are the Stratosphere, Mesosphere, and ...
... survive and our weather. The other three layers are the Stratosphere, Mesosphere, and ...
Chapter 13
... • Intense outward gas flows from surfaces • Occupy H-R diagram just above main-sequence ...
... • Intense outward gas flows from surfaces • Occupy H-R diagram just above main-sequence ...
Asymptotic Giant Branch
... • Most AGB stars (see later) and obviously also a large fraction of the RGB stars are variable • Variations in brightness, colour, velocity and extension observed • Possibility to „look“ into the stellar interior ...
... • Most AGB stars (see later) and obviously also a large fraction of the RGB stars are variable • Variations in brightness, colour, velocity and extension observed • Possibility to „look“ into the stellar interior ...
Ursa Minor
Ursa Minor (Latin: ""Smaller She-Bear"", contrasting with Ursa Major), also known as the Little Bear, is a constellation in the northern sky. Like the Great Bear, the tail of the Little Bear may also be seen as the handle of a ladle, hence the name Little Dipper. It was one of the 48 constellations listed by the 2nd-century astronomer Ptolemy, and remains one of the 88 modern constellations. Ursa Minor has traditionally been important for navigation, particularly by mariners, due to Polaris being the North Star.Polaris, the brightest star in the constellation, is a yellow-white supergiant and the brightest Cepheid variable star in the night sky, ranging from apparent magnitude 1.97 to 2.00. Beta Ursae Minoris, also known as Kochab, is an aging star that has swollen and cooled to become an orange giant with an apparent magnitude of 2.08, only slightly fainter than Polaris. Kochab and magnitude 3 Gamma Ursae Minoris have been called the ""guardians of the pole star"". Planets have been detected orbiting four of the stars, including Kochab. The constellation also contains an isolated neutron star—Calvera—and H1504+65, the hottest white dwarf yet discovered with a surface temperature of 200,000 K.