SLC Chemistry 1A/1AL Services: The SLC offers three services for students in Chem 1A/1AL this semester: Drop-in Tutoring (for Chem 1A/1AL), and Study Groups and Mock Exams (for Chem 1A only).Open the appropriate links below to find out more about each of these services.LC Chemistry 1A/1AL Services: The SLC offers three services for students in Chem 1A/1AL this semester: Drop-in Tutoring (for Chem 1A/1AL), and Study Groups and Mock Exams (for Chem 1A only).
After applying Newton's Laws of Motion and Newton's Law of Gravity we find that Kepler's Third Law takes a more general form: where M 1 and M 2 are the masses of the two orbiting objects in solar masses. Note that if the mass of one body, such as M 1, is much larger than the other, then M 1 +M 2 is nearly equal to M 1. In our solar system M 1 =1 solar mass, and this equation becomes identical to the first. Example: Phobos orbits Mars with an average distance of about 9380 km from the center of the planet and a rotational period of about 7hr 39 min. Use this information to estimate the mass of Mars.
There are two different formulas that you can use to find the axis of symmetry. One formula works when the parabola's equation is in vertex form and the other works when the parabola's equation is in standard form. If your equation is in vertex form, then the axis of is: x= h in the general vertex form equation y = (x-h) 2 + k. If your equation is in standard form, then the formula for the axis of symmetry is: $$ x = \frac {-b}{ 2a} $$ from the general standard form equation $$ y = ax^2 +bx + c $$.