使用节点前行和推力部署具有不同倾斜的星座
Shuailong Zhao1, Qinyu Zhu1, Xuefeng Tao1
1Graduate School, Space Engineering University, Beijing 101400, China.
Sensors (Basel, Switzerland)
|January 26, 2024
概括
选择正确的卫星星座部署策略是节省能源和时间的关键. 不同的推力类型 (脉冲与连续) 需要基于轨道倾斜的不同的方法来优化星座的位置.
科学领域:
- 太空飞船工程 太空飞船工程
- 轨道力学 轨道力学
- 任务设计 任务设计
背景情况:
- 星座部署任务需要仔细选择战略,以尽量减少能源消耗和时间成本.
- 部署策略的选择受使用的推力类型和所需的轨道特征的影响.
研究的目的:
- 研究和定义基于推力类型和倾斜的卫星星座部署的最佳策略.
- 在冲动和连续推力场景下,区分各种星座倾斜的部署方法.
主要方法:
- 对轨道元素 (倾斜,半长轴) 冲动推力效应的分析.
- 对轨道元素 (倾斜,半长轴) 的连续推力效应的分析.
- 基于每个推力类型的倾斜类别 (高,中低,中低,低) 的部署策略的分类.
主要成果:
- 冲动推力策略:对高倾斜的倾斜控制,对中低倾斜的半长轴控制.
- 连续推力策略:高倾斜的倾斜控制,中倾斜的半长轴控制,低倾斜的直接推力应用.
- 对于冲动和连续推进任务,制定了不同的战略选择标准.
结论:
- 最佳的卫星星座部署策略高度依赖于推力类型和目标轨道倾斜.
- 实施倾斜特定策略可确保对各种星座配置的有效能源和时间利用.
- 这项研究为在太空任务中选择有效的部署机动提供了一个框架.
相关概念视频
Rocket Propulsion in Gravitational Field - II
2.3K
A rocket's velocity in the presence of a gravitational field is decreased by the amount of force exerted by Earth's gravitational field, which opposes the motion of the rocket. If we consider thrust, that is, the force exerted on a rocket by the exhaust gases, then a rocket's thrust is greater in outer space than in the atmosphere or on a launch pad. In fact, gases are easier to expel in a vacuum.
A rocket's acceleration depends on three major factors, consistent with the...
A rocket's acceleration depends on three major factors, consistent with the...
2.3K
Circular Orbits and Critical Velocity for Satellites
2.9K
The Moon orbits around the Earth. In turn, the Earth (and other planets) orbit the Sun. The space directly above our atmosphere is filled with artificial satellites in orbit. One can examine the circular orbit, the simplest kind of orbit, to understand the relationship between the speed and the period of planets and satellites with respect to their positions and the bodies that they orbit.
Nicolaus Copernicus (1473-1543) first suggested that the Earth and all other planets orbit the Sun in...
Nicolaus Copernicus (1473-1543) first suggested that the Earth and all other planets orbit the Sun in...
2.9K
Rocket Propulsion in Gravitational Field - I
2.8K
Rockets range in size from small fireworks that ordinary people use to the enormous Saturn V that once propelled massive payloads toward the Moon. The propulsion of all rockets, jet engines, deflating balloons, and even squids and octopuses are explained by the same physical principle: Newton's third law of motion. The matter is forcefully ejected from a system, producing an equal and opposite reaction on what remains.
The motion of a rocket in space changes its velocity (and hence its...
The motion of a rocket in space changes its velocity (and hence its...
2.8K
Coriolis Force
3.4K
An accelerating particle experiences a force equal to the mass multiplied by the acceleration in an inertial frame of reference. Consider a particle in a non-inertial frame of reference, such as a sliding ball on a rotating table. The acceleration of the ball in this rotating reference frame is different than in the intertial frame, which modifies its equation of motion. The fictitious forces acting additionally on a rotating frame of reference alter Newton's Second Law expression.
3.4K
Non-uniform Circular Motion
7.2K
In uniform circular motion, the particle executing circular motion has a constant speed, and the circle is at a fixed radius. However, not all circular motion occurs at a constant speed. A particle can travel in a circle and speed up or slow down, showing an acceleration in the direction of motion. In that case, the motion is called non-uniform circular motion, and an additional acceleration is introduced, which is in the direction tangential to the circle.
For example, such...
For example, such...
7.2K
Kepler's Second Law of Planetary Motion
4.2K
In the early 17th century, German astronomer and mathematician Johannes Kepler postulated three laws for the motion of planets in the solar system. His first law states that all planets orbit the Sun in an elliptical orbit, with the Sun at one of the ellipse's foci. Therefore, the distance of a planet from the Sun varies throughout its revolution around the Sun.
While in an elliptical orbit, the total energy of the planet is conserved. Therefore, the planet slows down when it is at apogee and...
While in an elliptical orbit, the total energy of the planet is conserved. Therefore, the planet slows down when it is at apogee and...
4.2K


