The Sun is about 10.0 billion times brighter than the next brightest star, Sirius (as seen from Earth). How far would we have to be from the Sun for the Sun to be as bright as Sirius?
We would have to be ___× 10 5th AU or _____light-years away from the Sun.
The sun is 109 times brighter than Sirius, which has an apparent magnitude of -1.4. The apparent magnitude of the Sun is -26.7, while its absolute magnitude is 4.83. For the Sun to have a brightness as such as Sirius, it would have to have an apparent magnitude of-1.4. We can calculate the distance using the absolute and apparent magnitudes.
The distance of a star can be calculated if its absolute and apparent magnitudes are known,using the formula as shown below:
d = 10x10(m-M)/5
where m and M are the apparent and absolute magnitudes respectively.
Thus,
d = 10x10(-1.4-4.83)/5
d = 171.69pc
Thus, the Sun would have to be at a distance of 171.69 parsecs to appear as bright as Sirius.
The Sun is about 10.0 billion times brighter than the next brightest star, Sirius (as seen...
(a) The observed parallax of Sirius, the brightest star in the sky, is 0.375 arcseconds. How far away is it in parsecs? In light years? (b) The Hipparcos spacecraft could measure parallaxes as small as 0.001 a How distant is the furthest star for which we can measure parallax? How does this distance compare to the size of the galaxy!
A quasar has a brightness that corresponds to apparent magnitude 14.6 (Unit 55.4). a. If it is 1.29 billion pc away, how many times brighter than the Sun is it? The quasar is × 1011 times brighter than the Sun. b. How does this compare to the brightness of the Milky Way? Assume that the Milky Way contains about 1011 stars. The quasar is times brighter than the Milky Way.
According to Einstein’s formula, E=mc^2, the energy radiated away from the Sun (or any star for that matter) represents a loss in mass. That is, every Joule of energy radiated away from the Sun diminishes its mass by m=E/c^2. Assume that the Sun’s luminosity is 3.8X10^26 J/s. a) Determine the amount of mass (in kg) that the Sun would lose by shining at that same luminosity for 10 billion years. b) Sirius A will last about 90 million years as a...
1. What is your interpretation of "looking at distant objects only strictly tells us about their past, not the present" ? 2. Name and describe, in very simple terms, the three main methods we use to find/discover distant planets. 3. It is mentioned that if Sirius (the brightest of stars for us) indeed has the same intrinsic brightness of the Sun (as postulated by Huygens), but is observed by us as 600 million times fainter, it's distance should be about...
If we scale the approximate size of the Sun (~1 billion meters) to fit onto a DVD (about 100mm or 0.1m), how many DVDs would you have to connect as a chain to represent the distance to the nearest star? Use the fact that Alpha Centauri is about 10¹⁶ meters away from Earth. Hint: determine the scale factor which reduces the true size of the Sun to a DVD and apply it to the distance to Alpha Centauri. If you...
The light at the Earth from a certain star has an intensity of about 80.5×10-8W/m2. If the star emits radiation with the same power as our Sun, how far away is it from Earth? NOTE: Use 1000 W/m^2 as the intensity of the Sun at the Earth!
The light at the Earth from a certain star has an intensity of about 83×10-8W/m2. If the star emits radiation with the same power as our Sun, how far away is it from Earth? NOTE: Use 1000 W/m^2 as the intensity of the Sun at the Earth!
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. 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...
5. The HR Diagram. Suppose we consider a main sequence “O star” much more massive than the sun. According to the formulae shown in lecture: a. What is the luminosity of a main-sequence O star (in solar units, Lsun) of mass 100 solar masses? b. If the sun were a 100 solar mass main-sequence O star, how much brighter would it appear from the earth? c. What is the hydrogen fusing lifetime of this star in years? d. If the...
f) in vacuum, light travels at about 186,282 miles per second. One mile is about 161 kilometers (km). Astronomers prefer to use units of distance that are reasonable in describing how far objects are from Earth. For example, for distances in the solar system we use the astronomical unit (AU), which is equal to the average distance of Earth from the Sun; 1 AU is about 150 million km. For distances to stars and galaxies, astronomers use the light-year (1...