Final answer:
The unseen companion's classification depends on its mass: 3.4 Mo indicates a stellar mass black hole, 1.7 Mo suggests a neutron star, 13.5 Mo corresponds to a stellar mass black hole, 0.06 Mo is likely a brown dwarf, 000003 Mo points to a planet, and .8 Mo suggests a white dwarf. Option number C is correct.
Step-by-step explanation:
If you detect a companion of a star by the wobble—or greater motion—of that star using the Doppler Effect, but that companion is unseen, the companion's nature can be inferred from its mass:
- a. 3.4 Mo (solar masses)
The companion with a mass of 3.4 Mo is most likely a stellar mass black hole, as it exceeds the maximum mass for a neutron star which is around 2.2 Mo. - b. 1.7 Mo
The companion with a mass of 1.7 Mo is most likely a neutron star, as its mass falls within the range of 1.4-2.2 Mo for neutron stars. - c. 13.5 Mo
A companion with a mass of 13.5 Mo would also be classified as a stellar mass black hole due the mass being significantly greater than the maximum for a neutron star. - d. 0.06 Mo
A companion mass of 0.06 Mo suggests that it could be a brown dwarf, which has a mass between about 0.01 Mo and 0.07 Mo. - e. 000003 Mo
The companion with this tiny mass would most likely be a planet, as it is less than 0.01 Mo, which is the threshold beneath which objects are considered planets. - f. .8 Mo
A mass of .8 Mo would indicate a white dwarf, as the mass is within the range for white dwarfs of 0.3 to 1.4 Mo.