Stars Flashcards
What is one light year?
The distance light travels through space in one year
What is parallax?
Where the position of nearby stars appears to shift against the background of more distant stars as the earth moves around its orbit
What is one astronomical unit?
The mean distance between the centre of the sun and the centre of the earth
What is the parallax angle?
The angle subtended to the star by the line between the sun and the earth. It is also half the angler shift of the star’s line of sight over 6 months. Generally measured in arc seconds.
What is one arc second?
1 degree over 3600.
What is one parsec?
The distance to a star which subtends an angle of one arc second to the line from the centre of the earth to the centre of the sun.
What does a smaller parallax angle to a star mean?
The star is further away.
Describe the Hipparcos scale
A logarithmic scale to measure the magnitude of brightness of stars. A increase of 5 is a division of 100. Smaller number represent bigger magnitudes.
What is apparent magnitude?
A measure of brightness of a star that depends on the light intensity received from the star on earth.
What is the absolute magnitude of a star?
The star’s apparent magnitude if it was 10pc from earth
What is d measured in for the magnitude equation?
Parsecs
What is a blackbody?
A perfect absorber of radiation at all wavelengths and therefore emits a continuous spectrum of wavelengths. Eg. a star
Describe the blackbody radiation curve
y-axis is power radiated at each wavelength. x-axis is wavelength in micrometers. Visible range is about from 0.3 to 0.7 micrometers. Line curves up from near origin to peak wavelength then curves back down not as steep and levels off. Higher temperature blackbodies have a higher peak and a shorter peak wavelength.
Why can we assume a star is a blackbody?
Because any radiation incident on it would be absorbed and none would be reflected or transmitted by the star. Also, the spectrum of thermal radiation emitted by the star is a continuous spectrum with an intensity distribution that matches the shape of a blackbody radiation curve.
What is Wien’s displacement law?
The wavelength at peak intensity is inversely proportional to the absolute temperature of the photosphere of a star.
What is the photosphere of a star?
The light-emitting outer layer of a star. Sometimes called the surface of a star.
What is Stefan’s law
The total energy per second emitted by a blackbody (luminosity or power output) is proportional to its surface area, and its absolute temperature to the power 4.
Order of class of stars from hottest to coolest
OBAFGKM
Recite table of class of stars
See grid on specification
Why do spectra from stars contain absorption lines?
There is an atmosphere of hot gases above the photosphere. Atoms, ions and molecules of these gases absorb light photons of certain wavelengths emitted from the photosphere. The light that passes through these gases is therefore deficient in these wavelengths so its spectrum contains absorption lines.
What are Hydrogen Balmer lines?
The absorption lines on an emission spectrum from a star that correspond to excitation of hydrogen atoms from the n=2 energy levels to higher energy levels.
Why are Hydrogen Balmer lines only found in the spectra of O, B and A stars?
Other star’s are not hot enough for excitation of hydrogen atoms, due to collisions, to the n=2 state.
Why don’t hydrogen atoms in the n=1 state absorb visible photons?
Because visible photons don’t have enough energy to causes excitation from n=1.
Describe the Hertzsprung-Russel diagram
y-axis is absolute magnitude ranging from +15 up to -10. x-axis is temperature or spectral class ranging from 50k to 2.5k or OBAFGKM. Sun(G,+5). Main sequence band class B to M magnitude -10 to +15 and is straight, then levels, then straight with same gradient as start. Red giants(G-M,0to-5). White dwarfs(B-F,+15to+10).