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ASTRONOMICAL SOC IETY OF TASMANIA BULLETIN 160
ASTRONOMICAL SOC IETY OF TASMANIA BULLETIN 160

... made reflecting telescope in Seattle on the Pacific Coast of the U.S.A. also ...
Spectroscopic Investigation of Companion Stars in Herbig
Spectroscopic Investigation of Companion Stars in Herbig

... Herbig AeBe (HAEBE) binary systems are good environments for the study of pre-main sequence stellar evolution in companion stars whose mass may be significantly lower than that of the primary star. Measurements of the spectral type and surface gravity of the companion star in the system allow it to ...
Class 12 : Star formation I : The Interstellar Medium (ISM)
Class 12 : Star formation I : The Interstellar Medium (ISM)

Friday, August 29
Friday, August 29

... The Trouble with Angles • Angular size of an object cannot tell us its actual size – depends on how far away it is • Sun and Moon have very nearly the same angular size (30' = ½) when viewed from Earth ...
Summary Of the Structure of the Milky Way
Summary Of the Structure of the Milky Way

... The distances that appeared on the right are the distances to 10 randomly chosen stars from this map. They illustrate the point that even though we believe these stars to be most common, they are not good indicators of galactic structure because they cannot be seen at sufficient distances to resolve ...
astronomy - sfox4science
astronomy - sfox4science

... The four outer planets (Jupiter, Saturn, Uranus, and Neptune) are known as the “gas giants,” because they are much larger than Earth and are made almost entirely of gases. Since the gas planets have so much mass compared to the inner planets, they exert a much stronger gravitational force. Pluto is ...
The birth and life of stars
The birth and life of stars

...  The most massive pre–main-sequence stars take the shortest time to become main-sequence stars (O and B stars).  In the final stages of pre–main-sequence contraction, when hydrogen fusion is about to begin in the core, the pre–main-sequence star may undergo vigorous chromospheric activity that eje ...
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13 Space Photos To Remind You The Universe Is

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Planets and Stars Differences and Similarities

Word doc - UC-HiPACC - University of California, Santa Cruz
Word doc - UC-HiPACC - University of California, Santa Cruz

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answers2004_05_BC - Particle Physics and Particle Astrophysics
answers2004_05_BC - Particle Physics and Particle Astrophysics

...  almost all systems have only one giant planet, and very few indeed have more than 2 (cf. Jupiter and much smaller Saturn in solar system)  planets are discovered around stars with heavy element content similar to or higher than the Sun  spectral class is also similar to the Sun’s ...
lec03_30sep2011
lec03_30sep2011

... -~7% of solar-type stars have >Mj planets in the “terrestrial planet” region. Extrapolation of current incompeteness suggests >12% w/planets @ <20 AU. - multiple planetary systems are ~common - planetary resonances are ~common What can explain these properties? ...
Star Groups and Big Bang Power Point
Star Groups and Big Bang Power Point

...  Over half of all observed stars form multiple-star systems.  Binary stars are pairs of stars that revolve around each other and are held together by gravity. The center of mass, or barycenter, is somewhere between the two stars. ...
Earth Science 25.2A : Stellar Evolution
Earth Science 25.2A : Stellar Evolution

...  During their red giant phase, sun-like stars consume hydrogen and helium fuel at a fast rate.  Once this fuel is exhausted, these stars also collapse into white ...
The Milky Way`s Spiral Arms
The Milky Way`s Spiral Arms

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Required Project #1 Questions from “Guide to Using Starry Night Pro

... 1. How do the stars appear to move as the time changes in sidereal day units? a. from East to West b. from West to East c. from North to South d. from South to North e. they remain fixed 2. Now change the date to 2/4/2001 and turn off the daylight. With the time-step setting on sidereal day, you wil ...
Chapter 18 Notes - Valdosta State University
Chapter 18 Notes - Valdosta State University

... atoms. Since no space is taken up by electrons orbiting nuclei, the density of a neutron star is one billion tons per teaspoonful. A neutron star as massive as the Sun would be much smaller than the Earth. ...
Phys 100 – Astronomy (Dr. Ilias Fernini) Review Questions for
Phys 100 – Astronomy (Dr. Ilias Fernini) Review Questions for

... c. occurs when carbon and oxygen combine to form nitrogen, which produces energy. d. produces the energy responsible for bipolar flows. * e. combines four hydrogen nuclei to form one helium nucleus, which produces energy. 31. The region of the sun just below the photosphere a. is undergoing thermonu ...
Autumn - Dark Sky Discovery
Autumn - Dark Sky Discovery

Astrophysics 11 - HR Diagram
Astrophysics 11 - HR Diagram

... • These stars are called white dwarfs and lie in the bottom right hand corner of the HR diagram. • White dwarfs are stars at the end of their lives, where all of their fusion reactions have stopped and are they are just cooling down. ...
HW #8 Stellar Evolution I Solutions
HW #8 Stellar Evolution I Solutions

... Protostars emit mostly IR thermal radiation as they generate energy by converting gravitational potential energy into heat during collapse. The IR thermal radiation can pass through significant amounts of dust without attenuation. Thus, the dust is transparent to IR radiation and we can “see” the st ...
PHYSICS 1500 - ASTRONOMY TOTAL: 100 marks Section A Please
PHYSICS 1500 - ASTRONOMY TOTAL: 100 marks Section A Please

... Why does the bulge of a spiral galaxy appear yellow in colour? (a) All the blue starlight is scattered out of our line of sight. (b) The light is dominated by recombination radiation from HII regions. (c) Emission comes from elements in the interstellar medium heavier than ...
Brock physics - Brock University
Brock physics - Brock University

... 47. The electron neutrino (νe ) produced in hydrogen fusion in the core of the Sun can transform into the muon neutrino (νµ ) or tau neutrino (ντ ) as it travels through (a) the Sun’s interior with a high electron density. (b) the free space between the Sun and the Earth. (c) the Earth’s crust on it ...
Clues to the Origin of the Solar System
Clues to the Origin of the Solar System

... ! Sun, Jupiter, and Saturn have same hydrogen dominated composition implying they formed from the same materials. ! Terrestrial planets and satellites are deficient in light gases and ices. Formed too close to Sun for gases/ices to remain, leaving heavier rock and metal. ...
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Stellar kinematics



Stellar kinematics is the study of the movement of stars without needing to understand how they acquired their motion. This differs from stellar dynamics, which takes into account gravitational effects. The motion of a star relative to the Sun can provide useful information about the origin and age of a star, as well as the structure and evolution of the surrounding part of the Milky Way.In astronomy, it is widely accepted that most stars are born within molecular clouds known as stellar nurseries. The stars formed within such a cloud compose open clusters containing dozens to thousands of members. These clusters dissociate over time. Stars that separate themselves from the cluster's core are designated as members of the cluster's stellar association. If the remnant later drifts through the Milky Way as a coherent assemblage, then it is termed a moving group.
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