Absolute magnitude (AQA A-Level Physics): Flashcards

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Absolute magnitude
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Apparent magnitude (mm)

How bright a star appears from Earth

Absolute magnitude (MM)

Star brightness if at 10 parsecs from Earth

Standard distance for absolute magnitude

10 parsecs

Formula: mm and MM relation

mM=5log(d10)m - M = 5 \log(\frac{d}{10}), dd in parsecs

Definition of parsec

Distance where 1 AU subtends 1 arcsecond

1 parsec in light-years

3.26 light-years

1 parsec in metres

3.08×10163.08 \times 10^{16} m

Astronomical Unit (AU) value

1.50×10111.50 \times 10^{11} m

Parallax distance formula (dd in pc, θ\theta in arcsec)

d=1θd = \frac{1}{\theta}

Greater parallax angle means star is...

Closer to Earth

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