Even though the Earth has less mass than the Sun, the moon orbits Earth because it’s much nearer to it.
<u>Explanation
:</u>
The fact is that the Moon orbits both the Sun and the Earth. On looking at the orbit of the Moon, it orbits in the same manner the way Earth does, but in a Spiro graph pattern along with orbiting the Earth with a small wobble to it.
Since the Sun has greater distance from the Moon as compared to the Earth (around 400 times), the gravity of Earth draws better impact on the Moon.
The escape velocity of the Moon is about 1.2 km/s at the distance from the Earth which is not sufficient to get ripped away from the Earth.
Hence, the moon orbits the Earth along with orbiting the Sun together with the Earth, but seems as if it only orbits the Moon.
You can eliminate the answer A because the moon is super cold
For answer B, atmosphere is contained of gasses, not just oxygen alone
Definitely not C
The answer is D because the moon's gravity isn't strong enough to hold the gasses, as a result, only a small amount of gasses has an attraction to it ( the moon has a little atmosphere though) but not enough to be considered
Answer:
The separation distance between the parallel planes of an atom is hc/2sinθ(EK - EL)
Explanation:
The relationship between energy and wavelength is expressed below:
E = hc/λ
λ = hc/EK - EL
Considering the condition of Bragg's law:
2dsinθ = mλ
For the first order Bragg's law of reflection:
2dsinθ = (1)λ
2dsinθ = hc/EK - EL
d = hc/2sinθ(EK - EL)
Where 'd' is the separation distance between the parallel planes of an atom, 'h' is the Planck's constant, 'c' is the velocity of light, θ is the angle of reflection, 'EK' is the energy of the K shell and 'EL' is the energy of the K shell.
Therefore, the separation distance between the parallel planes of an atom is hc/2sinθ(EK - EL)
Answer:
Resistance increases with increase in temperature which depends on power supplied which also depends on voltage.
Thermal expansion will make resistance larger.
Explanation:
Light bulb is a good example of a filament lamp. If we plot the graph of voltage against current we will notice that resistance is constant at constant temperature.
The filament heats up when an electric current passes through it, and produces light as a result.
The resistance of a lamp increases as the temperature of its filament increases. The current flowing through a filament lamp is not directly proportional to the voltage across it.
tensile stress begins to appear in resistor as the temperature rises. Thus, the resistance value increases as the temperature rises. Resistance value can only decrease as the temperature rises in case of thin film resistor with aluminium substrate.
In case of a filament bulb, the resistance will increase as increase in length of the wire. The thermal expansion in this regard is linear expansivity in which resistance is proportional to length of the wire.
Resistance therefore get larger.
Answer:
![t'=1.1897*10^{-6} s](https://tex.z-dn.net/?f=t%27%3D1.1897%2A10%5E%7B-6%7D%20s)
t'=1.1897 μs
Explanation:
First we will calculate the velocity of micrometeorite relative to spaceship.
Formula:
![u=\frac{u'+v}{1+\frac{u'*v}{c^{2}}}](https://tex.z-dn.net/?f=u%3D%5Cfrac%7Bu%27%2Bv%7D%7B1%2B%5Cfrac%7Bu%27%2Av%7D%7Bc%5E%7B2%7D%7D%7D)
where:
v is the velocity of spaceship relative to certain frame of reference = -0.82c (Negative sign is due to antiparallel track).
u is the velocity of micrometeorite relative to same frame of reference as spaceship = .82c (Negative sign is due to antiparallel track)
u' is the relative velocity of micrometeorite with respect to spaceship.
In order to find u' , we can rewrite the above expression as:
![u'=\frac{v-u}{\frac{u*v}{c^{2} }-1 }](https://tex.z-dn.net/?f=u%27%3D%5Cfrac%7Bv-u%7D%7B%5Cfrac%7Bu%2Av%7D%7Bc%5E%7B2%7D%20%7D-1%20%7D)
![u'=\frac{-0.82c-0.82c}{\frac{0.82c*(-0.82c)}{c^{2} }-1 }](https://tex.z-dn.net/?f=u%27%3D%5Cfrac%7B-0.82c-0.82c%7D%7B%5Cfrac%7B0.82c%2A%28-0.82c%29%7D%7Bc%5E%7B2%7D%20%7D-1%20%7D)
u'=0.9806c
Time for micrometeorite to pass spaceship can be calculated as:
![t'=\frac{length}{Relatie seed (u')}](https://tex.z-dn.net/?f=t%27%3D%5Cfrac%7Blength%7D%7BRelatie%20seed%20%28u%27%29%7D)
(c = 3*10^8 m/s)
![t'=\frac{350}{0.9806* 3.0*10^{8} }](https://tex.z-dn.net/?f=t%27%3D%5Cfrac%7B350%7D%7B0.9806%2A%203.0%2A10%5E%7B8%7D%20%7D)
![t'=1.1897*10^{-6} s](https://tex.z-dn.net/?f=t%27%3D1.1897%2A10%5E%7B-6%7D%20s)
t'=1.1897 μs