The mass of the star hd 68988 is about 2.3 × 10³⁰ kg.
The mass of the star hd 68988 is about 1.16 times of our sun's mass.

<h3>Further explanation</h3>
Centripetal Acceleration can be formulated as follows:

<em>a = Centripetal Acceleration ( m/s² )</em>
<em>v = Tangential Speed of Particle ( m/s )</em>
<em>R = Radius of Circular Motion ( m )</em>

Centripetal Force can be formulated as follows:

<em>F = Centripetal Force ( m/s² )</em>
<em>m = mass of Particle ( kg )</em>
<em>v = Tangential Speed of Particle ( m/s )</em>
<em>R = Radius of Circular Motion ( m )</em>
Let us now tackle the problem !

<u>Given:</u>
mass of the sun = M_sun = 1.99 × 10³⁰ kg
radius of the orbit = R = 10.5 × 10⁶ km = 1.05 × 10¹⁰ m
Orbital Period of planet = T = 6.3 days = 6.3 × 24 × 3600 = 544320 seconds
<u>Unknown:</u>
mass of the star = M = ?
<u>Solution:</u>
<em>Firstly , we will use this following formula to find the orbital period:</em>














<h3>Learn more</h3>

<h3>Answer details</h3>
Grade: High School
Subject: Physics
Chapter: Circular Motion