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Related Concept Videos

Conditions of Equilibrium01:28

Conditions of Equilibrium

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Equilibrium refers to a state where a rigid body is not subjected to any translational or rotational motion. This state is achieved when the force and couple acting on a rigid body equal zero. When the system of external forces results in a net effect equivalent to zero, the rigid body is considered to be in equilibrium.
Internal forces are not considered for conditions of equilibrium because they occur in equal and opposite pairs within the body, effectively canceling each other. As a result,...
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Equilibrium Conditions for a Particle01:23

Equilibrium Conditions for a Particle

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When an object is in equilibrium, it is either at rest or moving with a constant velocity. There are two types of equilibrium: static and dynamic. Static equilibrium occurs when an object is at rest, while dynamic equilibrium occurs when an object is moving with a constant velocity. In both cases, there must be a balance of forces acting on the object.
To understand the concept of equilibrium, let us first consider the forces acting on an object. When different forces act on an object, they can...
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Dynamic Equilibrium02:20

Dynamic Equilibrium

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A reversible chemical reaction represents a chemical process that proceeds in both forward (left to right) and reverse (right to left) directions. When the rates of the forward and reverse reactions are equal, the concentrations of the reactant and product species remain constant over time and the system is at equilibrium. A special double arrow is used to emphasize the reversible nature of the reaction. The relative concentrations of reactants and products in equilibrium systems vary greatly;...
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Free Energy and Equilibrium02:56

Free Energy and Equilibrium

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The free energy change for a process may be viewed as a measure of its driving force. A negative value for ΔG represents a driving force for the process in the forward direction, while a positive value represents a driving force for the process in the reverse direction. When ΔGrxn is zero, the forward and reverse driving forces are equal, and the process occurs in both directions at the same rate (the system is at equilibrium).
Recall that Q is the numerical value of the mass action...
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Calculating Equilibrium Concentrations02:05

Calculating Equilibrium Concentrations

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Being able to calculate equilibrium concentrations is essential to many areas of science and technology—for example, in the formulation and dosing of pharmaceutical products. After a drug is ingested or injected, it is typically involved in several chemical equilibria that affect its ultimate concentration in the body system of interest. Knowledge of the quantitative aspects of these equilibria is required to compute a dosage amount that will solicit the desired therapeutic effect.
A more...
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Calculating the Equilibrium Constant02:46

Calculating the Equilibrium Constant

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The equilibrium constant for a reaction is calculated from the equilibrium concentrations (or pressures) of its reactants and products. If these concentrations are known, the calculation simply involves their substitution into the Kc expression.
For example, gaseous nitrogen dioxide forms dinitrogen tetroxide according to this equation:
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Conditions Affecting Social Space in Drosophila melanogaster
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Research on Star Sensor Imaging Simulation Under Near-Space Hypersonic Non-Equilibrium Flow Conditions.

Zhen Liao1, Hongyuan Wang1, Xi Cheng1

  • 1Research Center of Space Optical Engineering, Harbin Institute of Technology, Harbin 150001, China.

Sensors (Basel, Switzerland)
|February 13, 2026
PubMed
Summary
This summary is machine-generated.

This study developed a simulation model for star sensor imaging under hypersonic conditions. The model reveals that solid media radiation significantly degrades star sensor images, impacting performance on near-space platforms.

Keywords:
aero-optical effectshypersonic flowimaging simulationstar sensors

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Area of Science:

  • Aerospace Engineering
  • Optical Engineering
  • Astrodynamics

Background:

  • Star sensors are crucial for navigation in space.
  • Hypersonic flight conditions introduce significant challenges to imaging systems.
  • Degraded star sensor images hinder accurate attitude determination.

Purpose of the Study:

  • To develop a simulation model for star sensor imaging under hypersonic conditions.
  • To analyze the impact of thermochemical non-equilibrium flow on star sensor performance.
  • To provide theoretical support for star sensor design on hypersonic platforms.

Main Methods:

  • Utilized a two-temperature model for hypersonic non-equilibrium flow.
  • Simulated chemical reactions using Arrhenius law.
  • Quantitatively analyzed optical transmission and thermal radiation effects.
  • Simulated degraded star images under typical working conditions.

Main Results:

  • Thermochemical non-equilibrium flow significantly degrades star sensor images.
  • Radiation from solid media was identified as the primary degradation factor.
  • Detectable limit magnitudes were determined to be 3.28 and 4.55 under tested conditions.

Conclusions:

  • The developed model effectively simulates star sensor degradation under hypersonic conditions.
  • Solid media radiation is a critical factor affecting star sensor imaging.
  • Results offer vital support for designing and testing star sensors for near-space hypersonic applications.