I will mark brainliest!
Mark him brainliest! XD
(your welcome btw)
b. The Earth's surface receives less energy from the sun's rays.
c. The Earth's rotation transfers energy more evenly.
d. The Earth's atmosphere traps heat.
B. low enough to combine
C. low enough to overcome
D. equal to
E. great enough to overcome
Answer: E. great enough to overcome.
Explanation: The three phases of the substances are solid, liquid and gas.
When a substance is heated, that is the molecules gain kinetic energy as kinetic energy is directly proportional to temperature.
The phase change will take place only when kinetic energy will be greater than the inter molecular forces as the molecules have to move in more random motion.
For example: Solid with high inter molecular forces are heated to convert it into liquid state only when kinetic energy will overcome the inter molecular forces of attraction.
Answer:
4 kg m/s
Explanation:
According to the Law of Conservation of Momentum, the total momentum must be the same before and after a collision. The total momentum before the bat hit the ball was 12 kg m/s. After the collision, the ball has a momentum of 8 kg m/s. Therefore, the bat must have a momentum of 4 kg m/s.
Answer:what is the role of of geologist in the petroleum industry
A. Stay with the drillers to examine rocks and fossils brought to the surface.
B. Chart information on a well log
C. Calculate the distance and direction of movement of the lost vein of ore
D. locate environment in which the petroleum forms
Correct option. Is D locate environment in which petroleum forms
Explanation:
Petroleum geologists are usually linked to the actual discovery of oil and the identification of possible oil deposits or leads. It can be a very labor-intensive task involving several different fields of science and elaborate equipment. Petroleum
geologists look at the structural and
sedimentary aspects of the stratum/strata to identify possible oil traps
Answer: D locate environment in which the petroleum forms
Explanation:
Answer:
The centripetal acceleration of Deimos is .
Explanation:
The centripetal acceleration is defined as:
(1)
Where v is the velocity of Deimos and r is the orbital distance.
Notice that is necessary to determine the velocity first.
The speed of the Deimos can be found by means of the Universal law of gravity:
(2)
Then, replacing Newton's second law in equation 2 it is gotten:
(3)
However, a is the centripetal acceleration since Deimos almost describes a circular motion around Mars:
(4)
Replacing equation 4 in equation 3 it is gotten:
(5)
Where v is the orbital speed, G is the gravitational constant, M is the mass of Mars, and r is the orbital radius.
Finally, equation 4 can be used:
Hence, the centripetal acceleration of Deimos is .
The centripetal acceleration of Deimos, one of Mars' moon, can be calculated using its orbital period and distance from Mars. Convert the time units to seconds and use the formulas for velocity and centripetal acceleration to get an answer of approximately 7.84x10^-5 m/s^2.
To find the centripetal acceleration of Deimos, we can use the formula for centripetal acceleration, which is a =v^2/r , where v is the velocity and r is the radius (distance from Mars to Deimos). The velocity can be found using the formula v = 2πr/T, where T is the period (time for one complete orbit).
First, convert the days into seconds because the SI unit of time in physics is second. So, 1.26 days = 1.26 * 24 * 60 * 60 = 108864 seconds.
Then, calculate the velocity: v = 2 * π * 2.35x10^7m / 108864s = 1.36 km/s.
Finally, substitute v and r into the centripetal acceleration formula: a = (1.36x10^3m/s)^2 / 2.35x10^7m = 7.84x10^-5 m/s^2.
The centripetal acceleration of Deimos is approximately 7.84x10^-5 m/s^2.
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