By Richard Gates
When Alan Holt and I were
engineers in the aviation industry we enjoyed sailing Stars, built our own
equipment, and started Spar Tech Co. Alan had already established himself as a
talented Star sailor and continued to improve his performance in the Star
community. He has since left Spar Tech
and is pursuing his interest in windsurfing, growing grapes and making wine.
We have seen many
developments and changes in the Starboat spars over the years. There have been
fads, misunderstanding of the technical facts and real developments.
Wooden spars had wildly
differing weights, stiffness, and shapes.
When the Star Class established the tip weight limit and allowed the
aluminum spar, the characteristics of the Star mast homed in on a very narrow
variation of weights, stiffness, and shapes.
The Class officials did an excellent job of picking a reasonable tip
weight limit that has allowed the development of very good spars.
The
Development of Mast Sections
Since the 60’s, spar mast
refinements have been slow and intuitive – solid spruce, cedar cored spruce or
fir, elliptical aluminum section, teardrop sections, pointed front with blunt
aft section, and finally an aerodynamically designed section.
Each design evolution has
had distinct advantages; reduced overall weight, increases strength and
consistency, smaller section, increased stiffness reduced tip weight for same
stiffness, and finally an aerodynamically designed low drag configuration.
When the Class allowed
aluminum, the spar designers were a bit timid and inexperienced and the first
aluminum Star mast was an elliptical shape. Not a very exciting shape, but new
material made the bonfires after a windy race day a thing of the past.
As the spar builders and
designers gained experience, the favorite section became the 57 x 85 mm
teardrop shape. This shape had no
theoretical and/or experimental data to support its design. It just looked good to the eye. When this shape was introduced to the Star
Class in 1972, the current desktop computer power was a dream and computational
fluid dynamics programs did not include boundary layer effects.
With today’s powerful
desktop computers and sophisticated computational fluid dynamics (CFD) programs
it is possible to analyze the airflow about the Star jib, mast and mainsail
while taking the boundary layer effects into account.
In the later days of wooden
spars, competitors would do almost anything to save weight aloft – from hollow
tubes for bolts to ski poles for spreaders.
The introduction of the Class minimum tip weight set a lower limit for
the spars and allowed a structurally more conservative design, but the minimum
tip weight was still desired. Today,
some sailors are content to pay a tip weight penalty to achieve perceived
stiffness.
For a while some level
racing designs supposedly experimented with highly corrosive, high strength
alloys in an attempt to get stiffer spars for the same or reduced weight. This is not possible since the higher
strength alloys have the same modulus of elasticity and the same stiffness to
weight ratios. Fortunately the Class
had the vision to limit the allowable aluminum alloys to 90% aluminum which
prevents the use of many high strength, highly corrosive alloys.
Spar Tech wanted to improve
the aerodynamic characteristics of the Star mast and challenged Arvel Gentry,
(www.arvelgentry.com) a noted aerodynamicist who has worked with mast shapes
and sail/mast interaction, to investigate Star mast/sail interaction and design
a better mast shape. The only
constraints given to Arvel were the Star Class size limits, the requirement
that the external surface could not have any concavities, and the current sail
shapes. Arvel was free to design any shape that was aerodynamically superior.
The result of this extensive
study is the Spar Tech Company G section, Low Drag or GoLD mast. The GoLD mast section has near minimum tip
weight, improved aerodynamic performance, and bend properties to match existing
mainsails.
The knuckle on the forward corner is followed by a sloped and much flatter region that is faired into the maximum thickness point. This sloped region gives the boundary layer time to change from the laminar to the turbulent condition; and once the boundary layer is turbulent, it is able to stay attached further back on the mast before it separates. This is why golf balls have dimples. This is accomplished without concavities and/or trip devices.

The figure shows the
theoretical flow separation behind the GoLD Star mast when analyzed in the
presence of the jib and main sail. The
additional flow separation for the conventional teardrop section Star mast is
superimposed for reference. The
improvement is obvious and significant.
The result of the smaller separation region behind
the GoLD mast section is improved Lift/Drag characteristics for the mast, jib,
and main sails combination.

It was a rare opportunity for the Star Class to have
access to the expertise of Arvel Gentry and the CFD programs. Take advantage of what technology has to
offer:

A very detailed discussion of the GoLD mast design can be found at the web site www.spartechco.com.