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brilliants [131]
2 years ago
8

The distance from Earth of the red supergiant Betelgeuse is approximately 643 light-years. If it were to explode as a supernova,

it would be one of the brightest stars in the sky. Right now, the brightest star other than the Sun is Sirius, with a luminosity of 26LSun and a distance of 8.6 light-years. Part A How much brighter in our sky than Sirius would the Betelgeuse supernova be if it reached a maximum luminosity of 1.1×1010 LSun? Express your answer using two significant figures.
Physics
1 answer:
valkas [14]2 years ago
5 0

Answer:

1.5 Times.

Explanation:

The first step in order to solve the problem is to define our values, from this we can proceed to find the apparent brightness relationship for the two objects,

So,

B_i = \frac{L}{4 \pi R^2}

B=Apparent Brightness

L= Luminosity

R=Radius

Then,

\frac{B_{Berelgeuse}}{B_{Sirius}} = \frac{\frac{L_{Betelgeuse}}{4\pi (D_{Betelgeuse})^2}}{\frac{L_{Sirius}}{4\pi (D_{Sirius})^2}}

\frac{B_{Berelgeuse}}{B_{Sirius}} = \frac{\frac{1.1*10^{10}*L_{sun}}{4\pi (643)^2}}{\frac{26L_{Sun}}{4\pi(8.6)^2}}

\frac{B_{Berelgeuse}}{B_{Sirius}} = \frac{1.1*10^{10}}{643^2}*\frac{8.6^2}{26}

\frac{B_{Berelgeuse}}{B_{Sirius}} = 15682.3

B_{Betelgeuse} = 15682.3B_{Sirius}

Under this relationship we can conclude that in the case of a Supernova, in our sky Betelgeuse Supernova would be 1.5 * 10 ^ 4 times brighter than Sirius seen from the earth to the sky.

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Si el coeficiente de fricción cinética entre los neumáticos y el pavimento seco es de 0.80. ¿Cuál es la distancia mínima para de
vovangra [49]

Answer: 52.9 metros.

Explanation:

Podemos escribir la fuerza de fricción cinética como

F = μ*N

donde N es la fuerza normal entre el coche y el suelo, cuya magnitud es igual al peso en esta situación.

F = μ*m*g

donde m es la masa del coche y g es 9.8m/s^2

y sabemos que μ = 0.8

Por la segunda ley de Newton, sabemos que:

F = m*a

fuerza es igual a masa por aceleración.

a = F/m

entonces la aceleración causada por la fuerza de rozamiento es:

F = 0.8*m*g

a = F/m = (0.8*m*g)/m = 0.8*g.

Entonces ya encontramos la aceleración, hay que recordar que esta aceleración es en sentido opuesto a la sentido de movimiento, entonces podemos escribir la aceleración como:

a(t) = -0.8*g

Para la velocidad, podemos integrar sobre el tiempo para obtener.

v(t) = -0.8*g*t + v0

donde v0 es la velocidad inicial del auto = 28.7m/s

v(t) = -0.8*g*t + 28.8m/s

Ahora podemos encontrar el tiempo necesario para que la velocidad del coche sea cero, en ese momento, como deja de moverse, ya no tendremos rozamiento cinético, entonces no habrá aceleración y el coche se detendrá completamente.

v(t) = 0m/s = -0.8*9.8m/s^2*t + 28.8m/s

7.84m/s^2*t = 28.8m/s

                 t   = (28.8m/s)/(7.84m/s^2) = 3.63 segundos.

Ahora vamos a la ecuación de movimiento, donde asumimos que la posición inicial del coche es 0m, así que no tendremos constante de integración.

p(t) = -(1/2)*(0.8*9.8m/s^2)*t^2 + 28.8m/s*t

Ahora podemos evaluar la posición en t = 3.63 segundos, y esto nos dara la distancia que el coche se movio mientras frenaba.

p(3.63s) = -(1/2)*(0.8*9.8m/s^2)*(3.63s)^2 + 28.8m/s*(3.63s) = 52.9 metros.

6 0
2 years ago
A small charged sphere is attached to a thread and placed in an electric field. The other end of the thread is anchored so that
VMariaS [17]

Answer:

E = 9.66\times 10^{-6} N/C

direction is Horizontal

Explanation:

As we know that the string is horizontal here

so the tension force in the string is due to electrostatic force on it

now we will have

F = qE

so here the force is tension force on it

F = 6.57 \times 10^{-2} N

Q = 6.80 \times 10^3 C

now we have

6.57 \times 10^{-2} = (6.80 \times 10^3)E

E = 9.66\times 10^{-6} N/C

direction is Horizontal

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Answer:

false

Explanation:

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