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Binary Stars. a 3 P 2. M=k. X. Binary stars. orbit each other. Visual Binary Stars. 2 Conditions Required. Visual Binary Stars. 2 Conditions Required. 1-Far Apart. Visual Binary Stars. 2 Conditions Required. 1-Far Apart 2-Both Bright. 430pc. 25pc. Optical Double Stars.
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a3 P2 M=k X Binary stars orbit each other.
Visual Binary Stars 2 Conditions Required
Visual Binary Stars 2 Conditions Required 1-Far Apart
Visual Binary Stars 2 Conditions Required 1-Far Apart 2-Both Bright
430pc 25pc Optical Double Stars Look Like Visual Binaries Optical Illusion One Much Farther Away
March 1972 March 1982
Astrometric Binary Stars March 1972 March 1982
Astrometric Binary Stars March 1972 March 1982 What is required? Star Shows Measurable Motion in Few Decades Star Relatively Close to Us
a3 P2 M=k Astrometric Binary Stars March 1972 March 1982 March 1992 20 years = 1/3 P P = 60 years
Astrometric Binary Stars March 1972 March 1982 March 1992 a3 P2 M>k
Invisible Companion Not Bright Enough to Be Seen M=5M¤ M1=1M¤ M2=4M¤ Black Hole
Invisible Companion Not Bright Enough to Be Seen M=5M¤ M1=3.5M¤ M2=1.5M¤ Neutron Star Chandrasekhar Limit 1.4M¤
Invisible Companion Not Bright Enough to Be Seen M2<8%M¤ Brown Dwarf
a3 P2 M=k Astrometric and Visual Binary Stars Far Apart Both Bright Stars Shows Measureable Motion in Only a Few Decades Close to Us
Velocity Time Spectroscopic Binary
Spectroscopic Binary What is required? High Inclination
2pa P = v a3 P2 M=k Spectroscopic Binary v = v sin i
2pa P = v a3 P2 M>k Spectroscopic Binary v = v sin i
Invisible Companion Black Hole Neutron Star Brown Dwarf Planet
& Spectroscopic Binary Spectrum Binary B5 K2 Hot Cool What is required? Both Bright Different Temperature
Time Spectroscopic Binary Velocity
Eclipsing Binary Light Curve magnitude Time
Time Eclipsing Binary magnitude
Time Eclipsing Binary magnitude
Time Eclipsing Binary magnitude
Time Eclipsing Binary magnitude
Time Eclipsing Binary magnitude
Time Eclipsing Binary magnitude
Time Eclipsing Binary magnitude
Time Eclipsing Binary magnitude
Time Eclipsing Binary magnitude
Time Eclipsing Binary magnitude
Eclipsing Binary What is required? Both Bright Inclination = 90°
2pa P = v a3 P2 M=k Spectroscopic Binary v = v sin i
Time Eclipsing Binary magnitude
Time Eclipsing Binary magnitude
Star Sizes Surface Area = 4 p R2 Energy = s T4 Luminosity = 4 p R2s T4