Question

An M2 III RSG has an absolute visual magnitude (MV ) of approximately −0.6. (a) If...

An M2 III RSG has an absolute visual magnitude (MV ) of approximately −0.6.

(a) If this star were located in the globular cluster Omega Centauri what would be its apparent V magnitude? You will need to look up the distance of Omega Centauri.

(b) What would be the expected parallax of the star in Omega Centauri?

(c) Assuminga relativetangential velocity of 100kms−1, what is theexpected proper motion (in arcseconds/year) of the star in Omega Centauri?

Homework Answers

Answer #1

I have not done the MKS to Astronomical Unit transformation explicitly. You can derive the relation in part c very easily.

Know the answer?
Your Answer:

Post as a guest

Your Name:

What's your source?

Earn Coins

Coins can be redeemed for fabulous gifts.

Not the answer you're looking for?
Ask your own homework help question
Similar Questions
Consider a star with a parallax of 0.0073??, an apparent visual magnitude, V (= mV) of...
Consider a star with a parallax of 0.0073??, an apparent visual magnitude, V (= mV) of 10.4 mag and an absolute blue magnitude of MB = 5.8 mag. Assuming there is no extinction between us and it, determine the star’s: (a.) Distance. Report your answer in pc. (b.) Color index (B?V or MB ? MV). (c.) The Spectral Type and Luminosity class. Explain how you arrived at this answer.
The apparent magnitude of Sun in V filter band is -26.7 mag. Please answer what's the...
The apparent magnitude of Sun in V filter band is -26.7 mag. Please answer what's the absolute magnitude of the Sun in V-band? Suppose you are observing a globular cluster in the halo of the Milky Way, whose distance was 25 kiloparsecs, and you want to be able to detect stars like the Sun in this cluster. What would the apparent V magnitude be for a star identical to the Sun, if it were at that distance?
Vega is measured to have an apparent visual brightness of 3650×10−26 W/m2 /Hz and lies at...
Vega is measured to have an apparent visual brightness of 3650×10−26 W/m2 /Hz and lies at a distance of 7.7 pc from the Sun. (a) What flux would be observed if the star were moved to a distance of 2.0 kpc? (b) What flux would be observed if the star were moved to the Large Magellanic Cloud (LMC) which has a distance of approximately 52 kpc? (c) The apparent visual magnitude (V) of Vega is 0.03. What V magnitude would...
) Canopus (alpha Carinae) is the second-brightest star in the night sky, its apparent magnitude is...
) Canopus (alpha Carinae) is the second-brightest star in the night sky, its apparent magnitude is 0.7 m . Based on the parallax measurements of Hipparcos satellite, its parallax is approximately 0.01 arcseconds. (i) Find the distance to Canopus in parsecs and its absolute magnitude. [3 marks] (ii) Assuming that the absolute magnitude of the Sun is 4.8m show that the luminosity of Canopus in terms of the solar luminosity L⊙ is approximately 16000 L⊙. [2 marks] (iii) The emission...
Aldebaran is an orange giant star in the constellation Taurus. It has B, V , and...
Aldebaran is an orange giant star in the constellation Taurus. It has B, V , and R apparent magnitudes of B = 2.40, V = 0.86, and R = −0.37 respectively. Its bolometric correction mbol − mV = −0.6. (a) For a measured parallax angle of 0.0500, determine the distance to Aldebaran in pc. Also convert your answer to meters. (b) Determine the distance modulus to Aldebaran, and its absolute V magnitude. (c) Determine the ratio of Aldebaran’s luminosity to...