Introduction to Binary Stars Steve B. Howell NOAO.

Slides:



Advertisements
Similar presentations
Lecture 5 Binary stars.
Advertisements

7B Stars … how I wonder what you are.. 7B Goals Tie together some topics from earlier in the semester to learn about stars: How do we know how far away.
1. absolute brightness - the brightness a star would have if it were 10 parsecs from Earth.
Dr Matt Burleigh The Sun and the Stars. Dr Matt Burleigh The Sun and the Stars Binary stars: Most stars are found in binary or multiple systems. Binary.
Chapter 11 Surveying the Stars. I.Parallax and distance. II.Luminosity and brightness Apparent Brightness (ignore “magnitude system” in book) Absolute.
Binary Systems and Stellar Parameters The Classification of Binary Stars Mass Determination using visual Binaries Eclipsing,Spectroscopic Binaries The.
Binary stellar systems are interesting to study for many reasons. For example, most stars are members of binary systems, and so studies of binary systems.
Binary Stars Astronomy 315 Professor Lee Carkner Lecture 9.
Binary Stars Astronomy 315 Professor Lee Carkner Lecture 9.
The Properties of Stars Masses. Using Newton’s Law of Gravity to Determine the Mass of a Celestial Body Newton’s law of gravity, combined with his laws.
Intensity and Distance Intensity depends on luminosity and distance Inverse-square law discovered by Newton Magnitude system used in astronomy.
The Family of Stars Chapter 8:. Organizing the Family of Stars: The Hertzsprung-Russell Diagram We know: Stars have different temperatures, different.
Ch. 8 – Characterizing Stars part 3: The Hertzsprung-Russell Diagram Luminosity Classes Spectral Types.
Properties of Stars How do we measure stellar luminosities?
Properties of Stars. Distance Luminosity (intrinsic brightness) Temperature (at the surface) Radius Mass.
Astro 10-Lecture 9: Properties of Stars How do we figure out the properties of stars? We’ve already discussed the tools: Light Gravity (virtually impossible.
Surveying the Stars.
The Nature of the Stars Chapter 19. Parallax.
Chapter 11 Surveying The Stars Surveying The Stars.
The mass ratio of the stellar components of a spectroscopic binary can be directly computed from their ratio in radial velocities. To derive the total.
Chapter 13: Taking the Measure of Stars Stars come in a wide range of temperatures, sizes, masses and colors. The constellation of Orion is a good example.
AST 111 Exoplanets I.
Surveying the Stars Insert TCP 5e Chapter 15 Opener.
Universe Eighth Edition Universe Roger A. Freedman William J. Kaufmann III CHAPTER 17 The Nature of Stars CHAPTER 17 The Nature of Stars.
Chapter 10 Measuring the Stars. Units of Chapter 10 The Solar Neighborhood Luminosity and Apparent Brightness Stellar Temperatures Stellar Sizes The Hertzsprung-Russell.
ASTRO 101 Principles of Astronomy. Instructor: Jerome A. Orosz (rhymes with “boris”) Contact: Telephone:
1 II-6 Stellar Mass and Binary Stars (Main Ref.: Lecture notes; FK Sec.4 - 4, 6, 7; 17-9, 10, and 11, Box 4-2, 4-4) II-6a. Introduction If the star is.
Binary Stars. Double Stars/Binary Stars Binary Star Double Star Earth.
Measuring the Masses of Stars Binary Star Systems.
Properties of Stars.
Measuring the Mass of Stars Physics 113 Goderya Chapter(s): 9 Learning Outcomes:
BINARIES Read Your Textbook: Foundations of Astronomy
BINARY STARS How they help us to determine the mass of stars and the size of our galaxy.
Physical properties. Review Question What are the three ways we have of determining a stars temperature?
1 Stars Stars are very far away. The nearest star is over 270,000 AU away! ( Pluto is 39 AU from the Sun ) That is equal to 25 trillion miles! At this.
Lecture Outlines Astronomy Today 8th Edition Chaisson/McMillan © 2014 Pearson Education, Inc. Chapter 17.
The Nature of the Stars Chapter 19. Parallax.
Stars Stellar radii –Stefan-Boltzman law Measuring star masses.
Binary and variable stars. Students learn to: describe binary stars in terms of means of detection: visual,eclipsing, spectroscopic and astrometric.
Stellar Mass A star’s position on the main sequence is determined by mass. Mass and composition are set at a star’s birth.
Stars: Binary Systems. Binary star systems allow the determination of stellar masses. The orbital velocity of stars in a binary system reflect the stellar.
Solid Molecules Neutral Gas Ionized Gas (Plasma) Level of ionization also reveals a star’s temperature 10 K 10 2 K 10 3 K 10 4 K 10 5 K 10 6 K.
Binary Orbits. Orbits Binary Stellar Systems 1/3 to 2/3 of stars in binary systems Rotate around center of mass (barycenter) Period - days to years for.
Stars! A star is a big ball of gas, with fusion going on at its center, held together by gravity! Massive Star Sun-like Star Low-mass Star There are variations.
Stars come in all sizes, small, large and even larger.
Star Properties (Chapter 8). Student Learning Objectives Classify stars Explain how star properties are related.
Binary stellar systems are interesting to study for many reasons. For example, most stars are members of binary systems, and so studies of binary systems.
Binary Stars (Chapter 21 of book). The Types of Binary Stars Visual Binaries Eclipsing Binaries Spectroscopic Binaries.
Stars.
Copyright © 2010 Pearson Education, Inc. Lecture Outline Chapter 10 Measuring the Stars.
Binary stars and clusters Chapter 11. Review Properties of stars –apparent brightness (apparent magnitude) measure energy/area/second –luminosity (absolute.
Binary stellar systems are interesting to study for many reasons
PHYS 205 Multiple Star Systems PHYS 205 Binary systems Question: Why are the binaries important?? Answer: They allow us to measure the mass of other.
Three types of binary stars. Visual binaries – Stars that are far enough apart that they can be seen as separate stars through a telescope. They typically.
Remember that stellar distances can be measured using parallax:
Universe Tenth Edition Chapter 17 The Nature of the Stars Roger Freedman Robert Geller William Kaufmann III.
Properties of Stars. "There are countless suns and countless earths all rotating around their suns in exactly the same way as the seven planets of our.
11.2 Classifying Stars Our Goals for Learning How do we classify stars? Why is a star’s mass its most important property? What is a Hertzsprung–Russell.
Stellar Masses: Binary Stars
STELLAR MASSES AND THE HERTZSPRUNG-RUSSELL DIAGRAM
IB Physics Astronomy Elective
Binary Stars Hypothesis. Masses of Stars  While we can find the radius of a star from the Stefan-Boltzmann Law, we still do not know the mass  How do.
Binary Orbits.
Chapter 9: The Family of Stars
Binary Stars Palomar Observatory.
Stellar Mass.
Learning Goals: 4. Complex Knowledge: demonstrations of learning that go aboveand above and beyond what was explicitly taught. 3. Knowledge: meeting.
Binary stars and clusters
Stellar Masses.
Learning Goals: 4. Complex Knowledge: demonstrations of learning that go aboveand above and beyond what was explicitly taught. 3. Knowledge: meeting.
Presentation transcript:

Introduction to Binary Stars Steve B. Howell NOAO

Binary Stars ??

0 1

Binary Stars - Binary stars are pairs of stars orbiting each other connected by their mutual gravitational interaction. 50% of stars are binaries: ~100% O/B ~75% M Obs. biases

Binary Stars - Binary Stars may have orbital periods from seconds to hours to thousands of years They may contain stars of all kinds, sizes, and masses They may have circular or elliptical orbits They are believed to have formed together - same age (not capture) Close binaries affect each others evolution Long period binaries essentially act as single stars

Binary Stars - Types Binary stars come in a few types differentiated by their orbital period and/or observational behavior. For example: –Visual double (actually see both components - LONG period). Do not confuse with optical double –Astrometric binaries - see the wobble on the sky

Binary Stars - Types An astrometric and visual binary: Sirius A&B -- an A star (A) and a white dwarf (B) Has a ~50 year orbit. 8.6 light years from Earth Chandra Image

Binary Stars - Types or –Eclipsing binaries - one/two eclipses per orbit –Spectrum binaries - spectral properties change –Spectroscopic binaries - radial velocity motions (short periods easier to find)

Binary Stars - Types Schematic and real eclipsing binary light curves

Binary Stars - Types Spectral variations over time due to the binary nature of this star

Binary Stars - Types Or differentiated by other criteria- –Close binaries w/ stellar distortions or mass transfer –Intrinsic brightness changes due to stellar variability –Binaries with components of very different properties: color (WD+RD), mass (Exo- Planet), temperature –Other

Binary Stars - Types Binaries can be close (short orbital period) and show light variations due to … Ellipsoidal shape and/or tidal interaction Interactions such as mass exchange / transfer If the smaller (but more massive) star in an IB is a white dwarf, the binary is called a cataclysmic variable

Binary Stars - Types All combinations of the previous properties are possible Many are unknown as they simply have not been seen to vary (line of sight / observed) Binary Stars are the fundamental way in which we understand stars (and star systems): their formation, evolution & death. Remember --Three out of every two stars are in a binary system

Binary Stars - What can we learn? Eclipsing binaries are the best as the light curve can give stellar masses, radii, temperatures, & age estimates

Binary Stars - What can we learn? Eclipsing (or not) Radial velocity curve can give masses (or mass estimate) RV amplitudes give K1 & K2

Binary Stars - What can we learn? For a circular orbit Measure semi-major axis, a, from projected orbit & the distance. Relative positions about the center give: M1/M2 = a2/a1 = K2/K1 Keplers Law

Mass vs. radius and luminosity

The Oddest Eclipsing Binary? 1987 Epsilon Aurigae model from web site -->

The Oddest Eclipsing Binary Life?? Elemarkhorsaurus from the Epsilon Aurigae Binary Star System Caption: Ashraf, do you want to meet my new pet? Look, he is behind you and friendly. He loves the climate and his new home in the Eps Aur binary system. (From flickr)