3.9.2 Classification of stars Flashcards

1
Q

What is apparent magnitude?

A

The perceived brightness as seen from Earth

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2
Q

What is the Hipparcos scale?

A

A scale of apparent magnitude initially labelled 1.0-6.0, with 1.0 being the brightest, 6.0 being the dimmest

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3
Q

What is the relation between brightness and apparent magnitude?

A

In the Hipparcos scale, when apparent magnitude decreases by 1, brightness increases by 2.51 (100^(1/5))

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4
Q

What is a parsec?

A

The distance at which the radius of the Earth’s orbit (1AU) subtends an angle of 1 arcsecond

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5
Q

What is absolute magnitude?

A

The apparent magnitude of an object if it were placed 10pc away from Earth

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6
Q

What is Stefan’s law?

A

The output power of a black body radiator is directly proportional to its surface area and temperature^4
P=σAT^4.

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7
Q

What is Wien’s displacement law?

A

The peak wavelength of emitted radiation is inversely proportional to the absolute temperature of the object.
Tλ_max = constant

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8
Q

What is the general shape of black-body curves?

A

Peat at λ_max, then slopes down at the sides

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9
Q

What is assumed about a star when measuring its temperature (?)

A

Its a black body

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10
Q

What are the spectral classes?

A

O

B

A

F

G

K

M

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11
Q

What are Hydrogen Balmer lines?

A

Found in the spectra of O,B and A stars. They are caused by the excitation of hydrogen atoms from the n=2 state to higher/lower energy.

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12
Q

What is the parallax?

A

The apparent change of position of a nearer star in comparison to distant stars

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13
Q

How many light years are there in a parsec?

A

3.26

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14
Q

What are standard candles?

A

They are objects whose absolute magnitude is known and whose apparent magnitude can be measured.

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15
Q

What is a black body?

A

A body that absorbs all electromagnetic radiation of all wavelengths and can emit all wavelenghs of radiation

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16
Q

What is luminosity?

A

The total power output of a star (W)

17
Q

What is the brightness of a star?

A

The intensity of radiation received on Earth by the star (Wm^-2)

18
Q

What is the formula for the inverse square law of radiation?

A

I=P/(4πd^2)
For a given star, the luminosity is constant

19
Q

What does the inverse square law of radiation assume?

A

The source is treated as a point
The power from the source radiates uniformly through space
No radiation is scattered between the source and Earth

20
Q

What is AU?

A

Astronomical Unit: the average/mean distance between the centre of the Earth and the centre of the Sun

21
Q

What is a light year?

A

The distance travelled by light in a year

22
Q

What are the conversions for arcminutes and arcseconds?

A

1 degree = 60 arcminutes
1 arcminute = 60 arcseconds

23
Q

What is the absolute magnitude relationship?

A

m-M=5log(d/10)

M=absolute magnitude
m=apparent magnitude
d=distance of star from Earth (pc)

24
Q

What is the distance modulus?

A

m-M;
Used for determining the relative distance of a star.
Negative for stars closer than 10 pc
Positive for stars further away than 10 pc

25
Q

Which spectral classes have the strongest Balmer lines?

A

A- strongest
B - second strongest
O - weakest

26
Q

Describe the HR diagram

A

Supergiants at the top, giants at the top right, dwarves at the bottom, and main sequence stars forming a curve down the middle. Absolute magnitude on y-axis, 0 in the middle (corresponds to Sun), temperature on x-axis (40000K on left, 2500K on right)

27
Q

What is a binary system?

A

One where two stars orbit a common mass

28
Q

What are the 2 types of supernovae?

A

Type I; when a star accumulates matter from its companion star in a binary system and explodes after reaching a critical mass
Type II; The death of a high mass star after running out of fuel

29
Q

How can supermassive black holes form?

A

The collapse of massive gas clouds while the galaxy was forming
A normal black hole that accumulated large amounts of matter over millions of years
Several normal black holes merging together

30
Q

How did measurements not agree with Hubble’s law?

A

They found distant type 1a supernovae to be moving away from Earth at an increasing, speed, hence the universe is not expanding at a constant rate but accelerating.

31
Q

Why are supernovae used as standard candles?

A

Supernovae (occur at same critical mass, so have similar peak absolute magnitude), producing consistent light curves.