Yes the roational period around the Sun is likely to be getting faster since the dinosaurs were around.
From the Advanced Physics forums:
The Earth's orbit is eliptical, the amount it is out of round is only about 5,000,000 km in an orbit of radius about 150,000,000km. When you jump you push the Earth away from you slightly, but the difference in your mass and the Earth's mass is humungous. So the effect is very,very, small. However, there are people all over the Earth jumping at the same time, so the effects cancell each other.
There is also the pressure of sunlight on the Earth, and the moon. The Earth and the Moon are tied together by gravity so that it is their common centre of mass that orbits the sun. The orbit is decaying so in a few billion years the Earth will be closer to the sun. Meanwhile the Earth is slowing in its rotation and the day gets longer all the time. This is partly due to the drag of the tides.
By the way, space is a vacuum, there are only a couple of molecules per cubic meter.
PS
The sun is radiating alot of energy every day and e = mc^2 so its gravitational mass must be decreasing, causing our orbit to get very marginally bigger every second of every day!
http://curious.astro.cornell.edu/question.php?number=563
So the Sun loses 4,200,000,000 kilograms every second but it weighs 2 x 10^30 kilograms so that's a very small amount!
The Earth is also presumably slowing down as it collides with space dust as it travels through space every day - but given the Earth weighs alot more than dust, the collisions and decrease in speed is probably miniscule every century - so the effects maybe counterbalance!
PPS
http://www-istp.gsfc.nasa.gov/stargaze/Scalend.htm
Very precise atomic clocks nowadays tell us that the day is gradually getting longer. The culprits are the tides, twin waves raised in the Earth's ocean by (mainly) the Moon's gravitational pull. As the waves travel around the Earth, they break against shorelines and shallow seas, and thus give up their energy: theory suggests that this energy comes out of the (kinetic) energy of the Earth's rotational motion.
What then is the period of the Earth's rotation around its axis? A day, you say? Not quite.
Suppose we observe the position of a star in the sky--for instance Sirius, the brightest of the lot. One full rotation of the Earth is the time it takes for the star to return to its original position (of course, we are the ones that move, not the star). That is almost how the day is defined, but with one big difference: for the day, the point of reference is not a star fixed in the firmament, but the Sun, whose position in the sky slowly changes. During the year the Sun traces a full circle around the sky, so that if we keep a separate count of "Sirius days" and "Sun days", at the end of the year the numbers will differ by 1. We will get 366. 2422 "star days" but only 365. 2422 Sun days.
It is the "star day" (sidereal day) which gives the rotation period of the Earth, and it is about 4 minutes shy of 24 hours. A clockwork designed to make a telescope follow the stars makes one full rotation per sidereal day.
The clocks we know and use, though, are based on the solar day--more precisely, on the average solar day, because the time from noon to noon can vary as the Earth moves in its orbit around the Sun. By Kepler's laws (discussed in a later section) that orbit is slightly elliptical. The distance from the Sun therefore varies slightly, and by Kepler's second law, the motion speeds up when nearer to the Sun and slows down when further away. Such variations can make "sun-dial time" fast or slow, by up to about 15 minutes.
PPPS
http://www.lpi.usra.edu/education/skytellers/day_night.shtml
Good news for overachievers: Earth's days are getting longer!
Researchers examining ancient corals noted that annual growth patterns suggested there were more days in a year in Fossil corals from the Devonian Period (380 million years ago) recorded 400 daily cycles. About 290 million years ago in the Pennsylvanian Period, there were 390 daily cycles each year. Assuming that Earth's revolution around the Sun has not changed dramatically, this means that the number of hours per day has been increasing and that Earth's rotation has been slowing. Today, the length of a day is 24 hours. During the Pennsylvanian Period a day was ~22.4 hours long. In the Devonian Period, a day was ~21.8 hours long. Earth's rotation appears to be slowing approximately 2 seconds every 100,000 years. Why are Earth days getting longer? Some scientists suggest that tidal cycles create a "drag" on Earth, causing it to slow down.