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Sedbober [7]
2 years ago
3

A rogue black hole with a mass 12 times the mass of the sun drifts into the solar system on a collision course with earth. How f

ar is the black hole from the center of the earth when objects on the earth’s surface begin to lift into the air and ""fall"" up into the black hole? Give your answer as a multiple of the earth’s radius.
Physics
1 answer:
seropon [69]2 years ago
3 0

Answer:

Distance of blackhole from center of earth 2000 Re

Explanation:

we have mass of earth = Me = 5.972 \times 10^{24} kg

Mass of black hole Mb = 12 \times M_{sun} = 12 \times 1.989 \times 10^{30} kg = 23.868 \times 10^{30} kg

Object start to lift in air when net force on them becomes zero

\frac{ G Mb m}{x^2} = \frac{GM_{sun} m}{Re^2}

\frac{MB}{x^2} = \frac{M_E}{R_E^2}

x = \sqrt{\frac{Mb}{M_E}} R_E

x = \sqrt{\frac{23.868 \times 10^{30}}{5.972 \times 10^{24}}} R_E

x = 1.99 \times 10^{3} Re

x = 1999.16 Re

So, distance of blackhole from center of earth will be = x+ Re

     = 1999.16 Re + Re = 2000.16 Re

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Answer:

b ≈ 64 Kg/s

Explanation:

Given

Fd = −bv

m = 2.5 kg

y = 6.0 cm = 0.06 m

g = 9.81 m/s²

The object in the pan comes to rest in the minimum time without overshoot. this means that damping is critical (b² = 4*k*m).

m is given and we find k from the equilibrium extension of 6.0 cm (0.06 m):

∑Fy = 0 (↑)

k*y - W = 0    ⇒   k*y - m*g = 0   ⇒   k = m*g / y

⇒   k = (2.5 kg)*(9.81 m/s²) / (0.06 m)

⇒   k = 408.75 N/m

Hence, if

b² = 4*k*m    ⇒     b = √(4*k*m) = 2*√(k*m)

⇒     b = 2*√(k*m) = 2*√(408.75 N/m*2.5 kg)

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5 0
2 years ago
Sandra's target heart rate zone is 135bpm—172bpm. Marissa's target heart rate zone is 143bpm—176bpm. They stop playing basketbal
Feliz [49]

Answer: Neither Sandra nor Marissa will be in her THR zone.


Explanation:


1) Actual pulse of both Sandra and Marissa : 144 bpm


2) Decrease of 20 bpm ⇒ 144 bpm - 20 bpm = 124 bpm


3) Sandra's TRH is in the range 135 - 172 bpm.


Since 124 < 135, she will be below the range.


4) Marissa's TRH range is 143 - 176 bpm.


Since, 124 < 143, she is below the range


In conlusion, neither Sandra nor Marissa will be in her THR zone.

6 0
2 years ago
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One of the fundamental pillars to solve this problem is the use of thermodynamic tables to be able to find the values of the specific volume of saturated liquid and evaporation. We will be guided by the table B.7.1 'Saturated Methane' from which we will obtain the properties of this gas at the given temperature. Later considering the isobaric process we will calculate with that volume the properties in state two. Finally we will calculate the times through the differences of the temperatures and reasons of change of heat.

Table B.7.1: Saturated Methane

T_1 = 120K

p_1 = 191.6kPa

v_f = 0.002439m^3/kg

v_{fg} = 0.30367 m^3/kg

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v_2 = v_1

v_2 = 0.0783m^3/kg

Now from the same table we can obtain the properties,

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t = \frac{(145-273)-(120-273)}{5}

t = \frac{25}{5}

t = 5hr

Therefore the time taken for the methane to become a single phase is 5hr

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2 years ago
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Zanzabum

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p=\frac{I}{c}

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I=1000 W/m^2

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starting from the radiation pressure found at point (a), we can calculate the force exerted on a tritium atom:

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m=5.01\cdot 10^{-27}kg

we can find the acceleration, by using Newton's second law:

a=\frac{F}{m}=\frac{2.2\cdot 10^{-34} N}{5.01\cdot 10^{-27} kg}=4.4\cdot 10^{-8} m/s^2

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