Subscribe free to our newsletters via your
. 24/7 Space News .




TIME AND SPACE
Australian physicists cast new light on spin-bowling
by Staff Writers
London, UK (IOP) Jul 17, 2013


illustration only

As the Ashes series gets underway next week, a pair of brothers from Australia have been exploring the physics behind the spin of a cricket ball While physicists are much more accustomed to measuring the spin of electrons, protons and neutrons, Garry and Ian Robinson, Honorary Visiting Fellows at the University of New South Wales and the University of Melbourne respectively, have presented equations that govern the trajectory of a spinning ball as it moves through the air in the presence of a wind.

If the English and Australian cricketers are looking to take advantage of their results then they will be hoping that the unpredictable British weather brings plenty of wind throughout the five-game series, as the researchers have calculated that it can have a profound effect on the movement through the air of a spin-bowler's delivery.

According to the research, the presence of a cross-wind from either side of the cricket pitch can cause the spinning ball to either slightly "hold up" or "dip", depending on which direction the wind comes from and which way the ball is spinning. This therefore changes the point at which the ball pitches on the wicket.

Garry Robinson said: "Our results show that the effects on a spinning ball are not purely due to the wind holding the ball up, since a reversal of wind direction can cause the ball to dip instead. These trajectory changes are due to the combination of the wind and the spin of the ball.

"The effects of spin in the presence of a cross-wind, and how to fully exploit it, may or may not be completely appreciated by spin bowlers. Either way, we have provided a mathematical model for the situation, although the model of course awaits detailed comparison with observations."

As an example, the researchers show that when a 14 km/h cross-wind interacts with the spinning ball, the point at which it hits the ground can change by around 14 cm, which they believe may be enough to deceive a batsman.

The equations take into account the speed of the ball, gravity, the drag force caused by air resistance, and the Magnus or "lift" force, while at the same time incorporating the important effect of wind.

The Magnus force is a commonly observed effect, particularly in ball sports, when the spin of a ball causes it to curve away from its set path. This is observed in football when players purposely put spin on the ball to make it bend around a defensive wall.

Once the equations were constructed, they were numerically solved using a computer software program called MATLAB; the solutions were then used to create illustrative examples for cricket.

The researchers also show that a spinning cricket ball tends to "drift" in the latter stages of its flight as it descends, moving further to the off-side for an off-spinning delivery and moving further towards the leg-side for a leg-spinning delivery, effects which are well-known and regularly utilised by spin-bowlers.

"We hope that this work can be used to cast new light on the motion of a spinning spherical object, particularly as applied to cricket, whilst also stirring the interests of students studying differential equations," Garry continued.

The paper was been published 5 July, in Physica Scripta - a journal published by IOP Publishing on behalf of the Royal Swedish Academy of Sciences for the Science Academies and the Physical Societies of the Nordic Countries.

.


Related Links
IOP
Understanding Time and Space






Comment on this article via your Facebook, Yahoo, AOL, Hotmail login.

Share this article via these popular social media networks
del.icio.usdel.icio.us DiggDigg RedditReddit GoogleGoogle








TIME AND SPACE
Detection of single photons via quantum entanglement
Innsbruck, Austria (SPX) Jul 15, 2013
Almost 200 years ago, Bavarian physicist Joseph von Fraunhofer discovered dark lines in the sun's spectrum. It was later discovered that these spectral lines can be used to infer the chemical composition and temperature of the sun's atmosphere. Today we are able to gain information about diverse objects through light measurements in a similar way. Because often very little light needs to b ... read more


TIME AND SPACE
Soviet Moon rover moved farther than thought

Scientist says Earth may once have been orbited by two moons

Dust hazard for Moon missions: scientists

NASA Seeks Information on Commercial Robotic Lunar Lander Capabilities

TIME AND SPACE
New Mars mission: in the Vikings' steps

Overhead View of Mars Rover 10 Years After Launch

Third Drive of Curiosity's Long Trek Covers 135 Feet

DNA-sequencing chip could be sent to Mars to search for signs of life

TIME AND SPACE
The Zero Gravity Coffee Cup

Outside View: Future science fiction

New Flight Projects Building Boasts First NASA Goddard 'Green' Roof

Technology Could Curtail Astronaut Conflict

TIME AND SPACE
Medical quarantine over for Shenzhou-10 astronauts

China's astronauts ready for longer missions

Chinese probe reaches record height in space travel

China's space tracking ship Yuanwang-5 berths at Jakarta for replenishment

TIME AND SPACE
Space Station ARISS Software Upgraded by Student For Students

Astronaut's helmet leak forces abrupt end to spacewalk

NASA puzzled as astronaut's helmet leak halts spacewalk

Luca, the orbital repair man

TIME AND SPACE
Alphasat stacks up

ESA Signs Off On Baseline Configuration Of Ariane 6

Alphasat and INSAT 3D fueled for Ariane 5 heavy lift dual launch

Special group to be set up for inspecting production of Proton-M carrier rockets

TIME AND SPACE
UM Researchers Land NASA Grant to Search Space for Exoplanets

Disks Don't Need Planets to Make Patterns

Hubble Finds a Cobalt Blue Planet

Gaps in dust around stars may not indicate planets as many believe

TIME AND SPACE
Homemade 3D guns in US stir more buzz than bang

ASC Signal Doubles Mission Capabilities Across Its Satellite Antenna Line

Raytheon touts company developments

Surface porosity and wettability are key factors in boiling heat transfer




The content herein, unless otherwise known to be public domain, are Copyright 1995-2014 - Space Media Network. AFP, UPI and IANS news wire stories are copyright Agence France-Presse, United Press International and Indo-Asia News Service. ESA Portal Reports are copyright European Space Agency. All NASA sourced material is public domain. Additional copyrights may apply in whole or part to other bona fide parties. Advertising does not imply endorsement,agreement or approval of any opinions, statements or information provided by Space Media Network on any Web page published or hosted by Space Media Network. Privacy Statement