The intensity of an object is related to the distance d to the observer by the equation (I1/I2) = (d2/d1)2. If the apparent magnitude of the Sun seen from Earth has a value of -26.74, what is the apparent magnitude

of the Sun seen from Neptune (30AU from the Sun)?

To find the apparent magnitude of the Sun seen from Neptune, we can use the equation (I1/I2) = (d2/d1)², where I1 and I2 are the intensities of the Sun observed from Earth and Neptune, respectively, and d1 and d2 are the distances from the Sun to Earth and Neptune, respectively.

Let's use the apparent magnitude of the Sun seen from Earth (-26.74) to find the intensity ratio I2/I1.

The magnitude scale is logarithmic, and the relation between the difference in magnitudes (m1 - m2) and the ratio of intensities (I2/I1) is as follows:

(m1 - m2) = -2.5 * log(I2/I1)

Plugging in the values we have:

(-26.74 - m2) = -2.5 * log(I2/I1)

Let's solve this equation for log(I2/I1):

log(I2/I1) = (-26.74 - m2) / -2.5

Now we need to convert the intensity ratio back to the magnitudes:

I2/I1 = 10^(log(I2/I1))

Let's substitute the values we have and solve for I2/I1:

I2/I1 = 10^[((-26.74 - m2) / -2.5)]

Since we know that Neptune is 30 astronomical units (AU) away from the Sun, we can substitute d2 = 30 AU and d1 = 1 AU into the equation (I1/I2) = (d2/d1)²:

(I1/I2) = (30/1)²
(I1/I2) = 900

Now we can substitute I1/I2 = 900 into the equation I2/I1 = 10^[((-26.74 - m2) / -2.5)]:

900 = 10^[((-26.74 - m2) / -2.5)]

To solve for m2, we need to take the logarithm of both sides:

log(900) = log[10^[((-26.74 - m2) / -2.5)]]

Using the property of logarithms, we can bring the exponent down and simplify further:

log(900) = (((-26.74 - m2) / -2.5) * log(10))

Since log(10) = 1, we can simplify further:

log(900) = (-26.74 - m2) / -2.5

Now we isolate m2:

(-26.74 - m2) / -2.5 = log(900)

Let's solve this equation for m2:

-26.74 - m2 = -2.5 * log(900)

Finally, solve for m2:

m2 = -26.74 - (-2.5 * log(900))

By substituting the value of log(900) into the equation, you can determine the apparent magnitude of the Sun seen from Neptune.