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 60s, 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 todays 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.