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Hypersonic Frontiers

An exploration of speeds exceeding Mach 5, delving into the physics, challenges, and classifications of ultra-high-velocity flight.

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Introduction

Defining Hypersonic Speed

In the field of aerodynamics, hypersonic speed denotes velocities significantly surpassing the speed of sound. Conventionally, this regime begins at approximately Mach 5 and extends upward.[1][2] The precise Mach number demarcation is fluid, influenced by complex physical phenomena such as molecular dissociation and ionization, which become prominent around Mach 5 to Mach 10.[3] An alternative definition characterizes the hypersonic regime by the significant change in specific heat capacity with temperature, as the kinetic energy of the object is converted into thermal energy.

Kinetic Energy Conversion

A defining characteristic of hypersonic flight is the substantial conversion of kinetic energy into internal energy within the airflow. This process leads to significant increases in temperature, impacting the gas's properties. Unlike lower speed regimes where gas behavior can be approximated, at hypersonic velocities, phenomena like dissociation (breaking of molecular bonds) and ionization (creation of charged particles, forming plasma) become critical considerations.[3]

Characteristics of Hypersonic Flow

Shock Waves and Heating

Hypersonic flows exhibit distinct features compared to supersonic flows. A prominent characteristic is the formation of a shock layer, a region of highly compressed and heated gas immediately behind the shock wave.[1] The interaction between this shock layer and the vehicle's surface results in significant aerodynamic heating, a critical design challenge.[5][6]

Real Gas Effects

At the extreme temperatures generated during hypersonic flight, the gas no longer behaves ideally. Real gas effects become significant, including the vibrational excitation of molecules, their subsequent dissociation, and even ionization, leading to the formation of plasma. These non-equilibrium chemical processes dramatically alter the gas properties and heat transfer dynamics.[1]

Boundary Layer Dynamics

The conversion of kinetic energy into internal energy via viscous effects causes a significant increase in temperature within the boundary layer. This, in turn, leads to a decrease in density. Consequently, the boundary layer expands, potentially merging with the shock wave, especially near leading edges. This phenomenon, known as viscous interaction, complicates aerodynamic predictions.[1]

Mach Regimes Classification

Defining Flight Regimes

Aerodynamicists often categorize flight speeds into distinct regimes based on Mach number ranges, extending beyond simple subsonic and supersonic definitions. The transition into the transonic regime (around Mach 1) introduces complexities where airflow locally exceeds Mach 1, invalidating simpler aerodynamic theories. Hypersonic speeds (Mach 5+) introduce further complexities due to real gas effects and extreme heating.

The table below outlines the commonly recognized flight regimes, their approximate Mach number ranges, associated speeds, general characteristics, and examples of vehicles operating within them.

Regime Mach No. Speed (approx.) General Characteristics Aircraft Examples Missiles/Warheads Examples
Subsonic < 1 < 614 mph (988 km/h) Flow entirely below Mach 1. Rounded features, high-aspect-ratio wings. All commercial aircraft
Transonic 0.8–1.2 614–921 mph (988–1,482 km/h) Mixed subsonic/supersonic flow. Swept wings, supercritical airfoils. Flight range typically Mach 0.8 to Mach 1.3. Northrop X-4 Bantam (Mach 0.9)
Supersonic > 1 921–3,836 mph (1,482–6,173 km/h) Flow entirely supersonic. Sharp edges, thin airfoils, delta wings common. Starts above Mach 1.3. XB-70 Valkyrie (Mach 3), SR-71 Blackbird (Mach 3), Concorde (Mach 2), Tupolev Tu-144 (Mach 2)
Hypersonic > 5 3,836–7,673 mph (6,173–12,348 km/h) Significant aerodynamic heating, complex shock interactions, integrated designs required. Real gas effects begin. X-15 (Mach 6.7), X-43 (Mach 9.6), X-51 Waverider (Mach 5) BrahMos-II (Mach 8), Kh-47M2 Kinzhal (Mach 10), 3M22 Zircon (Mach 8-9), DF-ZF (Mach 5-10), HSTDV (Mach 6), Hwasong-8 (Mach 6-10)
High-Hypersonic [10–25) 7,673–19,180 mph (12,348–30,867 km/h) Thermal control is dominant. Ablative materials or heat-resistant skins needed. Blunt configurations often used due to heating. 53T6 (Mach 17), HTV 2 (Mach 20), Agni-V (Mach 24), DF-41 (Mach 25), M51 (Mach 25), Avangard (Mach 20-27)
Re-entry speeds ≥ 25 ≥ 19,180 mph (≥ 30,870 km/h) Ablative heat shields essential. Blunt shapes. Governed by atmospheric entry physics. Space Shuttle Orbiter (Mach 22), Buran, Boeing X-37 (Mach 25), Reusable experimental spacecraft (~Mach 25), IXV (Mach 22) Avangard (Mach 20-27)

Similarity Parameters

Simplifying Complexity

Analyzing the vast range of hypersonic conditions necessitates the use of similarity parameters. While Mach and Reynolds numbers are crucial for lower speeds, hypersonic flow requires additional parameters due to phenomena like the near-independence of oblique shock angles from Mach number at high speeds (M > 10) and the increasing importance of real gas effects.

Key Parameters

The product of the freestream Mach number ($M_{\infty}$) and the flow deflection angle ($\theta$), known as the hypersonic similarity parameter ($K = M_{\infty}\theta$), is a critical factor. For slender bodies, the slenderness ratio ($\tau = d/l$, where $d$ is diameter and $l$ is length) often replaces the deflection angle in similarity considerations.[9] Describing the gas state becomes complex, potentially requiring dozens of variables for non-equilibrium flows.

Flow Regimes

Perfect Gas Regime

This regime assumes the gas behaves ideally. Flow is still Mach number dependent, and simulations may require constant-temperature walls. This regime typically spans from Mach 5 (where ramjets become inefficient) up to Mach 10-12.[1]

High-Temperature Effects

As speeds increase, gases exhibit dissociation (molecular breakdown) and ionization (particle charging), forming plasma. Surface catalysis and the specific material of the vehicle's surface become important factors in heat transfer calculations. This regime begins around 2000 K and extends until ionization effects dominate.[1]

Radiation Dominated

Above approximately Mach 12 (around 12 km/s), heat transfer becomes primarily radiative rather than conductive. Modeling gases in this regime is exceptionally complex, especially when considering optically thick conditions where emitted radiation is reabsorbed within the gas. This represents the extreme end of hypersonic flight dynamics.

Related Concepts

Further Exploration

The study of hypersonic speed intersects with numerous advanced aerospace and physics concepts. Understanding these related areas provides a more comprehensive picture of high-velocity flight.

  • Hypersonic glide vehicles
  • Supersonic transport (SST)
  • Lifting bodies
  • Atmospheric entry dynamics
  • Hypersonic flight principles
  • Ramjet and Scramjet propulsion
  • Rocket engines
  • Plasma physics
  • Computational Fluid Dynamics (CFD)

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References

References

  1.  is generally debatable (especially because of the absence of discontinuity between supersonic and hypersonic flows)
A full list of references for this article are available at the Hypersonic speed Wikipedia page

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Important Notice

This content has been generated by an Artificial Intelligence model and is intended for educational and informational purposes only. It is based on data derived from publicly available sources, including Wikipedia, and may not reflect the most current or complete information.

This is not professional engineering or physics advice. The information presented should not substitute for consultation with qualified aerospace engineers, physicists, or other relevant experts. Always refer to authoritative technical documentation and consult with professionals for specific applications or design considerations.

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