Well now that I've done it once, it's pretty simple. Centrifugal acceleration is just q²r, where q is rotational speed and r is distance from the axis of rotation.
If you assume the centre of the Earth makes it around the sun once every 365.256 days, then its rotational speed is q = 2π/3.1558e7 rad/sec = 1.991e-7 rad/sec.
1 AU is 149,598,000,000 m (google) and the Earth's radius is rEarth = 6,400,000 m. We get two interesting distances-from-axis-of-rotation: rNight = 1 AU + rEarth = 149,604,400,000 m and rDay = 1 AU - rEarth = 149,591,600,000 m.
So the centrigugal force during the day is fDay = q²rDay = 0.0059299 m/s², and fNight = q²rNight = 0.0059304 m/s².
Thus total acceleration toward the center of the Earth is aDay = g + fDay = 9.8125798641 m/s² and aNight = g - fNight = 9.8007196285 m/s².
Therefore you are 1.0012101393 times as heavy -- or about 0.121% heavier -- during the day than you are during the night, due to the Earth's motion around the sun.
If we also take into account centrifugal acceleration due to the Earth's rotation, calculated earlier to be 0.034 m/s², then we get aDay' = aDay - 0.034 = 9.7786 m/s² and aNight' = aNight - 0.034 = 9.7667. The ratio comes out to be about the same, within four decimal places.
Probably you could test this if you found a heavy enough object whose weight wouldn't change between day and night (i.e. not an animal)...