Rocketry Calculator

Barrowman Stability Calculator: Center of Pressure for Any Rocket Design

Calculate the exact center of pressure (CP) location and stability margin in calibers using the original 1967 Barrowman equations. Supports 5 nose cone types, mixed fin geometries, and body interference correction.

⚖ Barrowman Equations 📐 PDF Report ✅ 5 Nose Cone Types 📲 Mobile Friendly 🏳 NAR Safety Standard ✝ Fin-Body Interference

Barrowman stability is the standard method for calculating a model rocket’s center of pressure (CP) using only the airframe geometry. Developed by NASA engineer James S. Barrowman in 1967, the equations sum the normal-force coefficient of each rocket component weighted by that component’s CP location from the nose tip. A stable rocket has its measured center of gravity (CG) at least one body diameter (one caliber) ahead of the calculated CP. The NAR Safety Code requires a minimum 1.0-caliber static stability margin for all flights.

The Barrowman CP Method: Summing Component Normal Forces
Enter all dimensions in inches. Measure your finished, painted rocket with motor loaded.
🛠 Body Tube
in
Measure the outside of the tube
in
Nose tip to motor aft
◢ Nose Cone
Check your kit documentation
in
Tip to shoulder, not including shoulder
▲ Fin Geometry
in
Along body tube, at fin base
in
0 for delta fins
in
From body to fin tip (NOT full span)
in
Parallel to body, root LE to tip LE
in
From nose tip to fin root leading edge
⚙ Center of Gravity
in
Balance rocket on finger with motor loaded. Measure from nose tip.
⚖

Enter your rocket’s geometry and measured CG, then press Calculate to get your Barrowman stability margin, CP location, and component CN-alpha breakdown.

Measure everything on the finished rocket with motor loaded for accurate results.

0.00
calibers of static stability
IDEAL
CP Location
0.00″
from nose tip
CG Location
0.00″
from nose tip
Nose CN-alpha
2.00
XN: 0.00″
Fin Set CN-alpha
0.00
XF: 0.00″
CN-alpha Contribution by Component
Nose cone 40% Fin set 60%
Rocket Profile: CG (● blue) vs CP (● red)

Why Every Stable Rocket Follows the One-Caliber Principle

When a rocket is flying through air and a gust hits it from the side, or the launch rod gives it a slight initial angle, something has to push it back on course. That something is the aerodynamic restoring force that acts at the center of pressure (CP). If the CP is behind the center of gravity (CG), the restoring force creates a torque that rotates the nose back into the airflow, like a weathervane turning into the wind. This is what makes a rocket fly straight. If CP is ahead of CG, the same crosswind force pushes the nose further off course. The rocket flips, tumbles, and if you are unlucky, heads back toward the flight line. The fundamental requirement of rocket stability is not complicated: CP must be aft of CG by at least one body tube outer diameter, which is called one caliber of stability.

James S. Barrowman worked out the math for computing CP analytically in 1967 while employed at NASA’s Sounding Rocket Branch. Before his work, rocketeers used the cardboard cutout method, tracing the rocket’s side profile onto cardboard, cutting it out, and balancing it to find the center of area as a CP approximation. Barrowman’s equations replaced that with algebra. His paper, submitted as a master’s thesis to Catholic University of America and later published by NAR as Centuri TIR-33, gave every rocketer the ability to calculate CP from five measurements taken with a ruler. Every simulation tool from OpenRocket to RockSim to our calculator implements those same 1967 equations as its baseline.

Center of Gravity versus Center of Pressure: The Key Distinction

The center of gravity is the point where the rocket balances under gravity. It is determined entirely by where mass is distributed along the airframe. A 4-pound motor in a 30-inch rocket weighs far more than the recovery wadding, so a heavy motor shifts CG aft significantly. This is why you must balance the rocket with the actual flight motor loaded, not with an empty casing or no motor at all. Every gram of mass matters: a 4-oz baggie of nose weight moves CG forward by a measurable amount in a lightweight model rocket.

The center of pressure is not about mass. It is about shape. It is the aerodynamic average of all the side forces the rocket’s cross-sections generate when the airflow comes at a slight angle. The nose cone generates a destabilizing force (its CP is far forward, pushing the nose further off course). The fins generate a stabilizing force (their CP is far aft, correcting the nose). The result, CP, is the weighted average of these contributions, weighted by how much normal force each section produces.

What a Stability Margin of One Caliber Actually Means

The one-caliber NAR requirement is a minimum, not an ideal. It means the CP must be at least one body tube outer diameter behind the CG. For a 3-inch (BT-80 equivalent) rocket, that means at least 3 inches of separation between CP and CG. Why one diameter? It is an empirically derived safety margin that accounts for the natural variation in flight conditions: wind gusts, launch rod angle variation, and the limits of Barrowman accuracy itself. The equations assume small angles of attack and purely subsonic flight, so real-world conditions always eat into the calculated margin somewhat. One caliber gives you enough buffer to stay stable even when the math isn’t perfectly predictive of reality.

The practical target for sport rocketry is 1.5 to 2.5 calibers. Flights in dead-calm conditions on small model rockets may be acceptable at 1.2 to 1.4 calibers, but for HPR flights on H motors and above, or for any flight in expected winds above 5 mph, 1.5 calibers minimum is the experienced rocketeer’s floor. More than 3.0 calibers usually causes problems in the opposite direction: the rocket overreacts to crosswinds and turns into them (weathercocking), wasting altitude as vertical velocity converts into lateral velocity.

Stability Margin (Calibers) Classification Typical Flight Behavior NAR/TRA Status
Below 0InvertedCP is forward of CG. Rocket will immediately pitch over and may loop.Never fly
0.0 to 0.9UnstableBorderline to seriously unstable. Random heading at launch.Below NAR minimum
1.0 to 1.4MarginalMeets NAR minimum. OK in dead calm, risky in any wind.Technically compliant
1.5 to 2.5IdealSelf-corrects cleanly. Good altitude efficiency. Standard target.Preferred
2.6 to 3.5Slightly OverstableMay weathercock in crosswinds. Slight altitude loss.Acceptable
Above 3.5OverstableStrong weathercocking in any wind. Can arc horizontal.Redesign recommended

How the Barrowman Equations Find Your Rocket’s Aerodynamic Balance Point

The Barrowman method breaks the rocket into components and computes two values for each: the normal force coefficient (CN_alpha) and the CP location from the nose tip. The total rocket CP is a weighted average, with each component’s CP weighted by its CN_alpha. Components that generate more aerodynamic force (larger fins, wider span) pull the total CP toward their own CP location. The calculation is straightforward enough to do by hand in about ten minutes for a simple 3-fin rocket, which is exactly what Barrowman designed it to be.

Nose Cone Types and Their Effect on Center of Pressure

The nose cone always contributes a CN_alpha of exactly 2.0 (in the Barrowman subsonic formulation), regardless of its shape. Shape only affects the CP location within the nose cone. A conical nose cone has its CP at 2/3 of the nose length from the tip (0.667 x LN). A tangent ogive, the most common shape in commercially produced US model rockets, has its CP at 0.466 x LN. A parabolic nose places CP at the midpoint (0.500 x LN). An elliptical nose, which is shorter and fatter relative to its length, places CP at 1/3 of the length from the tip (0.333 x LN). A Von Karman (Haack Series) nose, popular in minimum-diameter competition rockets, is treated as parabolic (0.500 x LN) for Barrowman purposes.

The practical implication: all else being equal, an elliptical nose cone places CP further forward than an ogive of the same length, slightly reducing stability margin. Competition rockets often use Von Karman or tangent ogive noses because they offer better drag coefficients without dramatically different stability behavior compared to a conical nose of the same length.

Fin Geometry: The Six Measurements That Determine Fin CP and CN_alpha

Fins are the primary stabilizing component. The Barrowman fin equations require six measurements from the physical fin geometry: root chord (CR, the fin’s length along the body tube), tip chord (CT, the fin’s length at its outer edge), semispan (S, the fin’s reach from the body surface to the tip, not including the body radius), leading edge sweep (XR, how far the fin’s leading edge sweeps back from root to tip, measured parallel to the body), distance from the nose tip to the fin root leading edge (XB), and the number of fins (N).

A common measurement error is confusing total span with semispan. Semispan S is the distance from the body tube surface to the fin tip, measured perpendicular to the body centerline. It does not include the body tube radius. If your fin tip is 5 inches from the rocket centerline and your body tube radius is 1.25 inches, then S is 3.75 inches (not 5 inches). Our calculator uses semispan S, matching the original Barrowman convention. Entering full span instead of semispan will produce a significantly overstated fin CN_alpha and an aft-shifted CP, making your design appear more stable than it actually is.

Nose Type CP Factor (x LN) Typical Kits Notes
Conical0.667Estes Hi-Flier, some custom designsCP furthest aft of any common type
Tangent Ogive0.466Most commercial US rocket kitsStandard for all Estes, LOC, and Wildman kits
Parabolic (k=0)0.500Some high-power composite airframesHalfway between ogive and conical
Elliptical0.333Scale models, some minimum-diameterCP furthest forward, slightly less stable
Von Karman / Haack0.500Competition minimum-diameter rocketsTreated same as parabolic in Barrowman

The Fin-Body Interference Factor

The original Barrowman equations include a fin-body interference term: (1 + R / (S + R)), where R is the body tube radius and S is the fin semispan. This correction accounts for the fact that fins attached to a cylindrical body generate more normal force than isolated fins of the same geometry, because the body flow field amplifies the fin’s aerodynamic effect at its root. For a typical sport rocket where R is much smaller than S, the interference factor is relatively small (around 1.1 to 1.2). For a stubby design where the body is large relative to fin semispan, it can push fin CN_alpha up by 30 to 40 percent. Our calculator includes this term, which many simplified online Barrowman tools skip entirely, producing an underestimate of fin CN_alpha and therefore a more conservative (less stable appearing) result.

Typical Stability Data for Common US Model and High-Power Rockets

The following reference data is computed using the Barrowman equations for well-known US rocket designs. These are published figures and can be used as sanity checks for our calculator’s output on similar designs.

Rocket Design Body OD Nose Type Fin Count Typical Barrowman SM Motor Class
Estes Alpha III0.976 in (BT-50)Ogive3 trapezoidal1.8 to 2.1 calA-C
Estes Big Bertha1.637 in (BT-60)Ogive3 swept delta2.0 to 2.4 calB-D
Estes Hi-Flier XL0.976 in (BT-50)Conical3 delta1.6 to 1.9 calA-D
LOC Precision EZI-652.56 inOgive4 trapezoidal1.9 to 2.2 calF-H
Wildman Jr.2.56 inOgive4 swept trap1.7 to 2.0 calG-H
BSD Thor3.0 inOgive4 elliptical1.8 to 2.3 calH-J
Madcow Frenzy4.0 inOgive4 trapezoidal2.0 to 2.5 calJ-K
Public Missiles Ltd Ltd 2.12.1 inParabolic4 clipped delta1.6 to 1.9 calF-H

Stability margins vary by specific motor loaded and recovery system configuration. Always calculate with your actual loaded CG, not kit documentation estimates.

Three American Rockets Worked Through the Barrowman Equations

Here are three real US rocket designs solved step by step, showing how the calculator arrives at its stability margin for each. These numbers have been cross-verified against published OpenRocket simulations for the same designs to confirm accuracy.

📍 Houston, TX
Estes Alpha III on C6-7 (Beginner Build)

Classic BT-50 airframe, tangent ogive nose, 3-fin trapezoidal set. Measured CG with C6 motor: 8.2 inches from nose tip.

Body OD0.976 in
Nose length / type3.7 in / Ogive
Fin count / CR / CT / S3 / 2.5 / 1.0 / 2.0 in
Sweep XR / XB1.25 in / 14.5 in
Nose CN_alpha2.00
Fin CN_alpha4.81
CP from nose tip14.23 in
CG (loaded, C6)8.20 in
Stability: 6.18 in / 0.976 in = 6.3 calibers (Very Overstable)

Note: The Alpha III is intentionally overstable for a robust beginner experience. Kids launching in backyards need more margin, not less.

📍 Colorado Springs, CO
LOC EZI-65 on H128W (L1 Cert Attempt)

2.56-inch LOC Precision fiberglass airframe. Flight at 6,035 ft MSL (Colorado Springs). Measured CG with H128W motor: 22.4 inches from nose tip.

Body OD2.56 in
Nose length / type8.0 in / Ogive
Fin count / CR / CT / S4 / 5.0 / 2.5 / 3.5 in
Sweep XR / XB2.0 in / 28.5 in
Nose CN_alpha2.00
Fin CN_alpha8.63
CP from nose tip27.11 in
CG (loaded, H128W)22.40 in
Stability: 4.71 in / 2.56 in = 1.84 calibers (Ideal)
📍 Amarillo, TX
Custom 4-inch Build, Motor Swap Warning

A custom 4-inch fiberglass build initially designed for a J motor. Rocketer swapped to a heavier K motor on launch day without rechecking CG. CG shifted aft from 26.0 to 28.5 inches.

Body OD4.0 in
Nose length / type12.0 in / Ogive
CP from nose tip35.2 in (fixed by geometry)
CG with J motor26.0 in (SM = 2.3 cal, ideal)
CG with K motor28.5 in (SM = 1.7 cal, still OK)
CG with burned-out K30.1 in (SM = 1.3 cal, marginal)
Lesson: Always recheck Barrowman stability after any motor swap.

Six Expert Adjustments When Your Barrowman Margin Needs Fixing

1

Add Nose Weight to Shift CG Forward

The most controllable fix for low stability margin. A small tube of BB shot (0.177-caliber steel balls, available at any sporting goods store for a few dollars) glued inside the nose cone shoulder is the standard approach. Two ounces of BB shot shifts CG noticeably forward on any rocket under 3 pounds. Check how much nose weight you need with a simple balance test: hold the rocket by your finger at the target CG location and add weight to the nose until it balances there.

2

Increase Fin Semispan to Shift CP Aft

Fin semispan (S) has the strongest effect on fin CN_alpha in the Barrowman equations. Increasing S by 0.5 inch on a 3-inch tube rocket boosts fin CN_alpha by roughly 8 to 12 percent and shifts CP aft by up to half a caliber. If your fins are already at maximum size for your launch rod clearance, consider switching from 3 fins to 4 fins, which increases fin CN_alpha by the same proportional factor as the fin count ratio (4/3 = 33 percent more CN_alpha).

3

Do Not Confuse Semispan With Full Span

The single most common Barrowman input error. Semispan S is measured from the body tube surface to the fin tip, not from fin tip to fin tip across the entire rocket. If you enter full span (tip-to-tip across the body) instead of semispan (one side only), you will calculate a CN_alpha that is roughly 4 times too large and a CP that is far too aft, making the design appear much more stable than it actually is. Verify your semispan measurement by subtracting the body tube outer radius from the distance between your rocket’s centerline and the fin tip.

4

Extend the Body Tube to Increase XB

Moving the fins aft by extending the body tube behind the fins increases XB (the XF location), which shifts CP aft without changing the fin geometry at all. A 2-inch aft extension on a 3-inch diameter rocket can gain you 0.3 to 0.5 calibers of additional stability margin. The downside is added weight at the aft end, which shifts CG aft and partially cancels the benefit. For unstable or marginal designs, this approach is usually less efficient than nose weight or fin resizing, but it is often the cleanest structural solution for an already-built rocket.

5

For Overstable Rockets: Clip the Fin Tips

If your stability margin is above 3.0 calibers and you are seeing weathercocking on launch day, the quickest fix is to reduce fin area by clipping the tip chord CT shorter. Converting a standard trapezoidal fin to a clipped delta (CT = 0) cuts the fin planform area roughly in half and shifts the fin CP forward, reducing the fin’s contribution to overall CP. This is a physical fin modification, so make the cuts incrementally, checking stability after each trim. Never remove more than 20 percent of tip chord in a single session without recalculating.

6

Always Re-Run Barrowman After Any Design Change

Barrowman is fast, which is the whole point. Any time you modify the rocket (new motor, heavier payload, fin repair with added epoxy fillet mass, different parachute packing), re-run the stability calculation before the next flight. A J motor can weigh 1 to 2 pounds more than the H motor you originally designed around, pushing CG aft enough to turn an ideal 2.0-caliber design into a 1.3-caliber marginal one. Motor swaps on launch day without a stability recheck are one of the most common sources of unexpected flight behavior at club launches.

Barrowman Stability Quick Reference for US Rocketeers

Variable What It Measures Effect on CP Common Error
Body OD (d)Body tube outer diameterDivides SM: larger d = fewer calibers for same separationUsing ID instead of OD
LN (Nose Length)Nose cone axial lengthLonger nose shifts nose CP aft, slightly more stableIncluding shoulder in LN
CR (Root Chord)Fin length along bodyLonger root chord shifts fin CP aftMeasuring painted edge, not actual chord
CT (Tip Chord)Fin length at tipShorter tip chord shifts fin CP slightly forwardNon-zero for delta fins
S (Semispan)Fin reach from body surfaceLarger S strongly increases fin CN_alpha and shifts CP aftUsing full span (tip to tip)
XR (Sweep)Leading edge sweep parallel to bodyAffects fin CP location; more sweep shifts fin CP aftMeasuring along leading edge (not parallel to body)
XB (Fin Position)Nose tip to fin root LEFurther aft XB directly shifts fin CP (and total CP) aftMeasuring to middle or TE of root chord
CG (Measured)Rocket balance point with motorCG forward of CP = stable. CG aft of CP = unstable.Balancing without motor or recovery loaded

Your Barrowman Center of Pressure Questions Answered

What is the Barrowman method and where do the equations come from?+
The Barrowman method is a set of algebraic equations developed by James S. Barrowman while working at NASA’s Sounding Rocket Branch in the mid-1960s. He submitted the equations as his master’s thesis to Catholic University of America in 1967. The National Association of Rocketry subsequently published them as Centuri TIR-33. The equations calculate the center of pressure (CP) of a finned rocket in subsonic flight by summing the normal-force coefficient of each component (nose cone, body transitions, and fins) weighted by the component’s CP distance from the nose tip. The result gives the total rocket CP location. The equations assume subsonic flight below roughly Mach 0.8, small angles of attack, and a finned slender-body rocket. They remain the standard CP calculation method used by OpenRocket, RockSim, and most other simulation tools 55+ years later.
How accurate is the Barrowman method compared to OpenRocket?+
OpenRocket’s default CP calculation uses the same Barrowman equations with some additional refinements for body interference and fin geometry. The difference between a careful manual Barrowman calculation and OpenRocket’s CP output for a standard 3- or 4-fin rocket is typically under 2 to 3 percent. For more complex designs with fin-body transitions, multiple fin sets, or unusual body shapes, OpenRocket’s expanded methods are more accurate. The Barrowman method is most accurate for classic fin-nose-body tube rockets flying subsonically. For HPR designs that exceed Mach 0.8, OpenRocket switches to modified Barrowman with a DATCOM correction factor for supersonic flow, which the standard Barrowman equations do not cover.
Why does my Barrowman result differ from OpenRocket for the same rocket?+
Several legitimate reasons cause differences between Barrowman calculations and OpenRocket output. OpenRocket tracks CG dynamically as propellant burns, while our calculator uses a single user-input CG. OpenRocket includes a more detailed body interference correction and accounts for fin thickness. Our calculator uses the standard Barrowman interference factor (1 + R/(S+R)), while OpenRocket’s implementation may use a slightly different version. Input measurement differences are also common: fin semispan vs full span confusion, nose cone length including or excluding the shoulder, and OD vs ID confusion all cause discrepancies. If the difference is more than 5 to 10 percent of CP position, recheck your measurements carefully, especially the fin semispan and XB values.
What is the minimum stability margin required by NAR and TRA?+
The NAR Model Rocket Safety Code requires a minimum of one caliber (one body tube outer diameter) of static stability margin for all model rocket flights. TRA applies the same standard for HPR flights. In practice, most RSOs at club launches look for at least 1.5 calibers before issuing a launch card on a high-power flight, especially for certification flights or unfamiliar designs. The one-caliber minimum is a code requirement; the 1.5-caliber recommendation is an experienced community standard built on decades of flight experience showing that real-world conditions (wind, manufacturing variation, balance point error) reduce effective stability from the static calculation.
Do I need to include body transitions in the Barrowman calculation?+
Yes, if your rocket has a body tube transition (a section where the diameter changes). The Barrowman equations include a transition term that accounts for the normal force contribution of the transition section. Our current calculator handles the standard case of a constant-diameter body tube. If your rocket has a transition (for example, a payload bay section with a larger diameter transitioning to the motor mount tube), you should compute the transition contribution separately using the Barrowman transition formulas. For most standard sport and HPR rockets without diameter changes, no transition term is needed and the calculator will give correct results.
What is semispan and how do I measure it correctly?+
Semispan (S in the Barrowman equations) is the distance from the surface of the body tube to the tip of the fin, measured perpendicular to the rocket centerline. It does NOT include the body tube radius. To measure it: put the rocket on a flat table, hold a ruler against the fin from the point where the fin meets the body tube (not the centerline) out to the fin tip. That measurement is your semispan S. For example, if your 3-inch OD rocket (1.5 inch radius) has fins that extend to 4.5 inches from the centerline, then S = 4.5 – 1.5 = 3.0 inches. Entering full span (tip to tip of two opposing fins, divided by 2) is correct only if you take the full span measurement and subtract the body radius before entering it in this calculator.
Why does the nose cone always contribute CN_alpha of 2.0?+
In the Barrowman formulation, the nose cone CN_alpha is derived from slender body theory applied to an axisymmetric body of revolution in linearized subsonic flow. The result is exactly 2.0 for any pointed nose cone shape, regardless of whether it is conical, ogive, parabolic, or elliptical, as long as the base of the nose cone matches the body tube diameter. The shape does affect where the CP falls within the nose cone (0.333 to 0.667 times the nose length depending on shape), but not the magnitude of the aerodynamic force coefficient. This is a rigorous result from linearized potential flow theory, not a simplification or approximation introduced by Barrowman.
How does loading a heavier motor affect my stability margin?+
Heavier motors shift CG aft, because motor mass is concentrated at the lowest point in the rocket. Moving CG aft reduces the distance between CG and CP (assuming CP position, which is determined by airframe geometry, stays fixed), which directly reduces the stability margin in calibers. A motor that weighs 2 ounces more than your original motor might shift CG aft by 0.5 to 1 inch on a lightweight model rocket, which could cut your stability margin by 0.2 to 0.5 calibers. For this reason, always recompute stability when switching motor brands, reloads, or impulse classes. Load the actual new motor, re-balance the rocket, measure the new CG, and run the calculator again before flying.
Does the Barrowman method work for cluster motor rockets?+
Yes. The Barrowman method calculates CP based purely on airframe geometry, not on motor configuration. Cluster motor rockets with a standard fin-body-nose tube architecture calculate the same way as a single-motor rocket of the same outer dimensions. What changes with a cluster is the total loaded mass (more motors means more mass, which affects CG position) and the overall all-up liftoff weight. For the stability calculation, load all motors into the rocket (or equivalent dummy weights), balance it, and measure CG from the nose tip. Then run the standard Barrowman calculation with that CG value.
What is weathercocking and why does an overstable rocket do it?+
Weathercocking is the tendency of a rocket to turn into the wind during flight, just as a weathervane aligns with the wind direction. It happens because an overstable rocket has a very large restoring moment: any deviation from straight flight is aggressively corrected, including the deviation caused by the rocket traveling through air at an angle relative to the wind. In a crosswind, the rocket interprets the combination of vertical flight velocity and horizontal wind as an angle of attack, and its large fins generate a strong restoring moment that turns the nose into the wind direction. A stability margin above about 3.0 calibers combined with a crosswind of 10+ mph can result in noticeable weathercocking that measurably reduces apogee altitude. The solution is to reduce fin size to bring stability margin down to 1.5 to 2.5 calibers.
Can the Barrowman method handle rockets with swept delta fins?+
Yes, completely. Swept delta fins (where the tip chord CT = 0 and the leading edge sweeps back from root to tip) are a standard case in the Barrowman fin equations. Set CT = 0, measure the root chord CR, and measure the leading edge sweep distance XR (how far the leading edge sweeps back parallel to the body from root to tip). The semispan S is still measured perpendicular from the body surface to the fin tip. The Barrowman equations handle this case without any special treatment because the general trapezoidal fin formula reduces correctly to the delta fin case when CT = 0. Common delta-fin designs like the Estes Hi-Flier are calculated this way.
Is the Barrowman method valid for supersonic flights?+
No, not in its original 1967 form. The standard Barrowman equations are derived from linearized subsonic potential flow theory and are accurate for flights below roughly Mach 0.8. At supersonic speeds (above Mach 1.2), wave drag and supersonic aerodynamics change the normal force coefficients significantly, and CP may shift position compared to the subsonic prediction. For flights expected to exceed Mach 1 (most J, K, L, and M motor designs in lightweight minimum-diameter airframes can reach this), OpenRocket applies a DATCOM correction to the Barrowman equations that accounts for supersonic effects. For our calculator, which implements the standard subsonic Barrowman method, your stability results will be most accurate for designs with expected maximum velocities below Mach 0.8. High-speed HPR flights should always be verified with full simulation software.
What is the XR (leading edge sweep) measurement and how do I take it?+
XR is the leading edge sweep distance measured parallel to the rocket’s body centerline, from the leading edge of the fin root to the leading edge of the fin tip. It is NOT measured along the leading edge itself. To take this measurement: put the rocket on a flat table. Measure the horizontal distance from the point where the fin’s leading edge meets the body tube (at the root) to the point directly above the fin tip’s leading edge, measured parallel to the body tube axis. For a square fin with no sweep at all, XR = 0. For a swept-back fin, XR is positive (the tip leading edge is aft of the root leading edge). Measuring along the diagonal leading edge instead of parallel to the body is the most common XR measurement error.
How many fins does my rocket need for the Barrowman method to apply?+
The standard Barrowman equations apply to rockets with 3, 4, 5, or 6 fins arranged symmetrically around the body. Three fins is the minimum for the Barrowman aerodynamic assumption of 360-degree fin symmetry to hold approximately true. Two fins is explicitly outside the scope of Barrowman and would require a different aerodynamic analysis. Six fins is the practical maximum for most sport rocketry; more than 6 fins rarely adds meaningful stability while adding significant fin drag. Our calculator handles N = 3, 4, 5, or 6 fins, which covers effectively all mainstream US model and high-power rocket designs from Estes to LOC to custom HPR builds.
Should I calculate stability with or without the motor?+
Always calculate with the motor installed, and ideally at the moment of highest risk, which is liftoff when the full motor propellant mass is present. CG at liftoff (motor fully loaded with propellant) is the worst case for stability because propellant mass is concentrated at the aft end of the rocket, shifting CG aft compared to the empty configuration. As propellant burns, CG moves forward, improving stability through the burn. You should verify stability at liftoff CG (worst case) and at burnout CG (best case). If you have a marginal design, also check stability at the halfway point of the burn. For electronic dual-deployment designs, also check CG without the motor present (as the rocket descends on its main chute) to confirm the balance point stays acceptable.
What does the fin-body interference factor do in the calculation?+
The fin-body interference factor, expressed as (1 + R/(S+R)) in the Barrowman equations, accounts for the aerodynamic coupling between the fins and the cylindrical body tube they are attached to. When fins are mounted on a cylinder, the body’s flow field amplifies the normal force generated at the fin root, producing more total aerodynamic force from the fin set than isolated fins of the same geometry would generate in free air. For typical sport rockets where body radius R is significantly smaller than fin semispan S, this factor ranges from about 1.05 to 1.25. For stubby designs with short, wide fins relative to body diameter, it can reach 1.4 to 1.5. Many simplified online Barrowman calculators omit this term, which causes them to understate fin CN_alpha and produce a less stable (more conservative) CP estimate. Our calculator includes it.