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Stars & Planets - Introduction - 1) General Knowledge on Stars
Which is the most abundant element in the Universe ?
Iron
Oxygen
Hydrogen
Helium
Carbon
Where/How was Helium first discovered ?
In Cleveite
With radioactivity
In the solar spectrum
All the elements where produced during the Big Bang.
non
oui
Why do stars shine ?
Because they are hot.
Because they are cool.
Because of the nuclear reaction in their core.
What is roughly the temperature at the center of the Sun ?
15'000 K
1'500K
15 x 10^6 K
15 x 10^9 K
Massive stars live longer than low-mass stars.
non
oui
What is the approximate lifetime of the Sun ?
10 million years
4.5 billion years
10 billion years
20 billion years
The Sun will end its life as a
Neutron star
Supernova
White Dwarf
A type Ia Supernovae is the explosion of
A massive stars
A white dwarf
Betelgeuse is a
White dwarf
Red dwarf
Red Supergiant
Where is/was Hydrogen produced?
During the Big Bang
In Stars
In the interstellar medium
Lead (Pb) is produced by
Nuclear fusion
Cosmic ray spalliations
Neutron capture
Which are the most numerous stars
Stars of the mass of the Sun
Stars 10 times more massive than the Sun
Stars 10 times less massive than the Sun
Who discovered the Pulsars?
Jocelyn Bell Burnell
Albert Einstein
Margareth Burbridge
Which of these can be used as standard candles to measure extra-galactic distances?
Red supergiants
White Dwarfs
Cepheids
Type Ia Supernovae
Type II Supernovae
According to Planck's law, the spectral distribution of a thermal energy radiated by a black body (i.e. the pattern of the intensity of the radiation over a range of wavelengths or frequencies) depends
its temperature only
its temperature and brightness
The Hertzprung-Russel diagram shows
the luminosity of stars vs their mass
the luminosity of stars vs their effective temperature
the mass of stars vs their effective temperature
What is the so-called Kelvin-Helmoltz timescale for stars?
An estimate of how long a star can shine without nuclear reaction.
An estimate of how long it takes for a star to collapse with no internal pressure.
Université de Genève