21 Flashcards

(40 cards)

1
Q

What reaction powers the Sun’s core?

A

Nuclear fusion in the core.

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2
Q

What is the basic fusion reaction formula?

A

nucleus 1 + nucleus 2 → nucleus 3 + energy.

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3
Q

Why is energy released during fusion?

A

Because the mass of products is less than the mass of reactants.

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4
Q

What equation relates mass and energy in the Sun?

A

E = mc².

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5
Q

What is the rest energy formula?

A

E₀ = mc².

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6
Q

What is an electron volt (eV)?

A

A unit of energy equal to the energy gained by an electron when accelerated by 1 volt.

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7
Q

How much energy is 1 eV in Joules?

A

1 eV = 1.602 x 10^-19 J.

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8
Q

What is the energy equivalent of 1 atomic mass unit (amu)?

A

1 u = 931.5 MeV/c².

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9
Q

What is the Q-value in nuclear reactions?

A

The amount of energy released or absorbed in a nuclear reaction.

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10
Q

What is the Q-value of 2H + 3H → 4He + n?

A

17.5 MeV.

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11
Q

Why must nuclear fusion occur at high temperatures?

A

High temperatures overcome the electrostatic repulsion between protons.

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12
Q

What is the first step in the PP chain?

A

p + p → D + e⁺ + neutrino.

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13
Q

What is the final step in the PP chain?

A

He-3 + He-3 → He-4 + 2p.

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14
Q

What is the net result of the PP chain?

A

4 protons → He-4 + energy + 2 neutrinos + 2 positrons.

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15
Q

What is the % of mass converted to energy in hydrogen fusion?

A

0.71% of the mass is converted into energy.

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16
Q

How much energy is released per 1 kg of hydrogen burned?

A

6.38 x 10¹⁴ J/kg.

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17
Q

How many kg of hydrogen does the Sun consume per second?

A

6 x 10¹¹ kg/s.

18
Q

How much energy is released in a single PP chain reaction in joules and MeV?

A

4.287 x 10^-12 J = 26.7 MeV.

19
Q

How much helium is produced per second in the Sun?

A

596 million tons of helium per second.

20
Q

How much mass is converted to energy per second in the Sun?

A

4 million tons converted into energy per second.

21
Q

What is the luminosity of the Sun?

A

L = 3.85 × 10²⁶ W.

22
Q

What is the solar constant?

23
Q

What surface area receives 500 W on Earth from sunlight?

A

A body with surface area 0.5 m².

24
Q

What is the energy production per kg of the Sun over its lifetime?

A

3 × 10¹³ J/kg over 5 billion years.

25
How does the Sun maintain hydrostatic equilibrium?
By balancing gravitational collapse with outward pressure from fusion.
26
What is the solar core's density?
150,000 kg/m³ (20 times iron).
27
How is energy transported within the Sun?
Via radiation in inner zone, convection in outer zone.
28
What is the photosphere?
The Sun’s visible surface, granulated due to convection.
29
What causes sunspots and what is their temperature effect?
Strong magnetic fields lower temperature, appearing dark.
30
What is the sunspot cycle and its duration?
An 11-year cycle of sunspot increase and decrease.
31
What are solar prominences and solar flares?
Prominence = slow gas loop, flare = fast explosion of energy.
32
What is the solar wind and how does it escape the Sun?
Through coronal holes, visible in X-rays.
33
What is the solar corona and when is it visible?
Visible during solar eclipse when photosphere is blocked.
34
What are the physical properties of the Sun (mass, radius, temp, etc.)?
Mass = 2x10³⁰ kg, Radius = 700,000 km, Temp = 5800 K, Luminosity = 4x10²⁶ W.
35
What star is used to compare to the Sun and what are its properties?
Star Vega: 2.1 M☉, 2.4 R☉, 1.66 T☉, 40 L☉.
36
How many Earths can fit in the Sun?
About 1 million Earths.
37
What is the Sun's rotation period and how does it vary?
27-30 days, depending on latitude.
38
What energy output is equivalent to the Sun’s luminosity?
10 billion 1-Mton bombs per second.
39
How much energy does the Sun produce per second?
4 x 10²⁶ W.
40
What is the total energy output of the Sun over 5 billion years?
3 x 10¹³ J/kg.