In 2000, extrasolar planets with masses comparable to the mass of Saturn were first detected around the stars HD 16141 (also called 79 Ceti) and HD 46375. Search the Web for information about these planets. How do their masses compare to previously discovered extrasolar planets? Do these planets move around their stars in the same kind of orbit as Saturn follows around the Sun? If not, explain the differences.
Already registered? Login
Not Account? Sign up
Enter your email address to reset your password
Back to Login? Click here