Orbiting trajectory

 

 During the propelled phase, the launcher follows a law of attitude which will gradually bring it in the direction required for the injection of the satellite.

  During the flight, the trajectory is constantly recalculated taking into account the trajectory actually followed by the launcher.

 

The departure is done vertically to cross the atmosphere as quickly as possible and as the density of the atmosphere decreases, it will leave the vertical direction which is the direction in which gravity is exercised.

  The reduction of speed undergone by the rocket on a vertical course is expressed by the formula 9,81 x t

 Using the slingshot effect

 

  The earth makes a complete turn on itself in 24 hours

V = 2 π R cos (L) / 24

• R: Radius of the Earth in km (6378)

• L: Latitude of the point in degree

t: Time in days

• V: Speed in km / h

 At the poles, the speed of rotation is zero. At the equator, it is 465 m / s. Thus, before taking off, the satellite already has 5.7% of the speed needed for a low orbit.

 

For Kourou, this speed is 463 m / s,

For Cape Canaveral 410 m / s (inclination of 28.5 °)

For Baikonour of 323 m / s (inclination of 45.6 °).

 

That is why we throw more often towards the east and from a site placed near the equator. To avoid that the rocket falls on inhabited areas it is necessary to the west of the site an ocean or a desert. It is preferable that this ocean or desert also open to the North or South for launching into polar orbits.

 Choice of inclinations

The slingshot gain is only effective for a launch in equatorial orbit.

If the target orbit is inclined, this velocity will only be partly useful (proportion determined by trigonometry).

For a polar orbit, it is useless, the latitude of the launch site will be almost indifferent

If, the launch is retrograde (towards the west), the rotation of the ground penalizes the shot because it is necessary to compensate this speed.

 

For a site far from the equator, it is best to choose an orbit whose inclination is about the latitude of the site.

 

Orbiting can be done in two different ways depending on the target injection point.

If the target orbit is low, passing close to the launch site, it is possible to ignite all the stages one after the other.

If, on the other hand, the target orbit is high or if the orbital plane is very far from the launch site, then ballistic phases are inserted during the powered phase.

 

Ariane space launches its satellites directly into the transfer orbit GTO (Geostationary Transfer Orbit). Shots are fired from Guyana 5.23 ° north of the equator by successive lighting of its three floors.

 

For a GTO orbit, it is necessary to add to the satellite in addition to its apogee engine, a perigee engine for injection.

Rocket guidance

The first rockets were not guided: once launched, they followed a ballistic trajectory.

This is the case for the last stages of some space launchers, for rockets, and micro-rockets (amateur rockets, fireworks).

 

  To achieve an objective, or to place a satellite in orbit, it is necessary that this rocket is guided, that is to say that it can modify its trajectory and control its roll.

 

  Orders are obtained by a system of gyroscopes or by guidance from the ground.

 

Aerodynamic guidance

Flaps with movable flap, (at least 3). By turning the flap in one direction, a force is created in one direction or the other, perpendicular to the axis of the rocket. This force turns it around its center of gravity. Aerodynamic control also helps control roll. This system can only be used in the atmosphere.

Dans le cas d'un lanceur multi-étage, ce n'est utilisable que pour le premier étage qui évolue dans l'atmosphère.

Les missiles qui ne quittent pas atmosphère emploient ce système, seul ou avec tuyère orientable.

 

Nozzle flow deflection method

 

Sometimes the injection of liquid or gas into the nozzle is used to deflect the flow of gas. If a stage has at least two nozzles, it is only to steer them differently to have roll control.

If there is only one, we have the choice between 3 solutions:

-V verniers, small auxiliary engines

For liquid propellant engines, a small portion of the gases produced to power the turbopump are used.

-Aerodynamic control (for a first floor).

- A system of valves on the flanks of the rocket.

 

Orbiting

A satellite revolves around a star with such a speed that the centrifugal force compensates for its weight. It is therefore pseudo-isolated, so its speed remains constant as long as it is out of the atmosphere.

 

The satellite is not weightless. He is even constantly falling, but thanks to his speed, he falls and misses the Earth.

The speed given to a satellite decreases with the altitude of this one:

The higher he is, the less he is subject to gravity. The speed of orbiting is 8 km / s at 200km and 6.9 at 2000 km. The real problem in getting into orbit is not to climb, but to give the payload the desired speed.

 

GROUND DISTANCE

CIRCULAR SPEED

RUNTIME OF REVOLUTION

 

200 km

 

7,86 km/s

        

 

1 h 28

280 km

 

7,75 km/s

 

1h 30

 

573 km

 

7,58 km/s

 

1h 36

 

1688 km

 

7,04 km/s

 

2 h

 

4191 km

 

6,15 km/s

 

3 h

 

6426 km

 

5,59 km/s

 

4 h

 

10400 km

 

4,88 km/s

 

6 h

 

20255 km

 

3,87 km/s

 

12 h

 

35900 km

 

3,07 km/s

24 h

 

 It is not easier to place a satellite in a distant orbit than in a nearby orbit, since it requires less speed.

 

  The characteristic speed of an altitude of 4.88 km / s and 10400 km altitude is much higher than that of a 7.86 km / s and 200 km altitude orbit.

The most economical way to place a satellite in an orbit far from the Earth is the transfer.

transfert

 

Specialisations of the orbit

Whether elliptical or circular, an orbit is characterized by:

1 The period T (time for a revolution) which is calculated by the third law of Kepler. This period T depends only on the half-major axis. It will be 90 minutes for a satellite at 200 km altitude and 24 hours to 36 000 km.

2 The altitude is in km.

3 The inclination to the equator. If the latter is close to 0 °, the orbit is called equatorial, if it is close to 90 °, it is polar.

4 The apogee (highest point) the greatest distance to the earth

5 The perigee (the shortest distance)

6 The perigee argument: An angle between the apogee and perigee line with the Equator plane (less than or equal to the inclination of the orbit). An ellipse has two homes. An ellipse of string x and of foci A and B (x> AB) is the set of points M such that MA + MB = x.

7 The precession of the apse line: The axis connecting apogee and perigee (line of the apses) of an inclined elliptical orbit also turns around the axis of the poles.

 

The orbit of a satellite will be circular only if its injection takes place, on the one hand parallel to the ground, and on the other hand at the right altitude for a given speed. If these conditions are not met, the orbit is elliptical.

caracteristiques

The GEO orbit

The geosynchronous orbit has a period of revolution of 23 h 56 min 4s, the sidereal period of rotation of the earth. According to the inclination of this orbit, the satellite will describe "8" in the sky more or less elongated according to the inclination.

The geostationary satellite has the property of remaining fixed with respect to a ground observer. Its orbit is equatorial, circular and synchronous with the rotation of the earth.

 

The third law of Kepler shows that the altitude of such an orbit is 35,786 km, the satellite travelling at a speed of 3.074 km / s.

This type of orbit is used for telecommunication satellites and most weather satellites.

 

To access it, the satellite is placed in an elliptical orbit whose apogee is 36000 km. By going to the climax, we give a gas blow to reach the final orbit.

 

For the satellite to remain well in its orbit, it is necessary to adjust its trajectory which limits its lifespan to 7-10 years. Small control engines make it possible to make corrections. The sun and moon also cause disturbances of the order of 1 ° per year.

These satellites because of their altitude are almost permanently outside the cone of shadow of the earth and thus benefit from constant illumination. During the equinox period (March and September), they can sometimes be plunged every day in the dark for periods not exceeding 72 minutes.

Orbit SSO (Sun Synchonous Orbit) or sun-synchronous orbit.

The satellite in its orbit suffers disturbances due to the nearby land.

Since it is not spherical and its mass is not uniform, gravitational variations disturb the trajectory of the satellite.

 

If we want the plane of the orbit to keep a constant orientation with respect to the sun, we must rotate it a little less than 1 ° per day (360 ° / 365 days).

 

The satellite remains exposed to the sun, above the penumbra (evening / morning). Some Earth observation satellites are placed in such orbits, and they have always seen on a lit ground (with the light inclined, so shadows highlighting the reliefs).

 

This illumination also benefits the solar panels of the satellite that are constantly lit in the same way. Such a satellite placed on an orbit at 830 km, inclined at 98.7 °, will fly over a territory always at the same solar time. Likewise, it will fly over an area for a period of 26 days.

The transfer The transfer is a more complex spatial positioning than the orbiting.

But a satellite rotating around the Earth at 7.86 km / s, in a circular orbit, 200 km above sea level.

If at a point at this altitude, instead of this speed of 7.86 km / s we give it 8.72 km / s, it will go up to a climax located at 4 191 km.

With 9.42 km / s, it will reach an apogee located at 10 400 km. With 10.38 km / s, it will go up to an apogee located at 35900 km. By slightly increasing the circular velocity at one point in the orbit, the trajectory is lengthened.

 

When the satellite is at the apogee of its new trajectory, at an altitude of 4191 km, it can be traced in circular orbits at this altitude. But the speed remaining at the satellite at the peak of the elliptical orbit is less than the circular velocity corresponding to that altitude.

This remaining speed is:

5.43 km / s at the peak of 4 191 km.

3.69 km / s at the peak 10 400 km.

transfert1.39 km / s at the peak of 35900 km.

 

It is therefore 0.72 km / s, 1.19 km / s 1.68 km / s, respectively, for the satellite to establish itself in its new circular orbit.

 

The speed boost will be provided by a rocket engine installed on the satellite and directing its jet towards the rear of its course, and creating a thrust forwards.

Hohmann transfer orbit

A trajectory (also called transfer) of Hohmann is a trajectory that allows to go from a low circular orbit to another higher circular orbit located in the same plane, using only two impulse manoeuvers. By limiting itself to two manoeuvers, this trajectory is the trajectory consuming as little energy as possible

 

Whether losing a certain amount of speed or gaining it, whether the transfer is negative or positive, the satellite's manoeuvering rockets have exactly the same energy to develop.

manoeuvre 

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Placement into geostationary orbit GTO

 

Telecommunication satellites (satellite television) are placed in a geostationary transfer orbit (GTO). It is an elliptical orbit, with an apogee at 36000 km altitude and a perigee at (200 km).

The rocket propels the satellite to 200 km with a speed of 10.2 km / s. This speed is greater than that of orbiting (8 km / s), it moves away from the circular orbit and loses speed (like a glider that rises). It arrives at 36000 km (peak of its orbit) and it remains only a speed of 1.6 km / s. He must use his own engine of apogee to gain a little speed (from 1.6 to 3 km / s) and circularize its orbit. Some rockets (proton and future American rockets) can launch directly in GTO.

 

Fuel is reserved to correct changes in the orbit by solar winds. The circularization motor is always the one that then performs the corrections.

The correction system must be liquid propellant because it must be turned on a large number of times). When he runs out of fuel, he is out of order.

To avoid cluttering the orbit, the newer use their last fuel reserves to deviate.

 The lifespan of a geo satellite is 10 to 15 years.

But if the shot is made from a site far from the equator, you have to do more detours. If you shoot from a center far away from the equator, the satellite must use a large amount of fuel to make a "turn". Its life is diminished.

There is no difference between the launching of an inhabited ship and that of an ordinary satellite, except for a difference in weight and accuracy.

 

Back to earth

 

The manned space ship, to return to earth performs maneuvers.

Unlike the launch, if we reduce the circular speed, the satellite will shorten its trajectory.

At 200 km altitude, the orbit is near the first dense layers of the atmosphere. A slowdown will make it sink into the atmosphere to be destroyed by combustion in the atmosphere.

An inhabited ship must be designed on the contrary not to be destroyed.

Return to the atmosphere consists of a braking out of the atmosphere, and a braking in the atmosphere and a stabilization of the vessel.

The orbit on which the inhabited ship is travelling is determined by its speed of orbiting.

The voluntary slowdown must be obtained by a reaction system, by a rocket ejecting gases

It is necessary that the rocket is directed forward "retro-rocket".

 

At 200 km altitude, a loss of speed of 60 m / s would be enough to shorten the trajectory of 200 km, if the atmosphere did not exist, the satellite, after half a turn, would come tangent the earth.

The energy capable of slowing down a satellite by 60 m / s is exactly the same as that which could have given it a speed of 60 m / s.

 

According to Tsiolkovsky's equation: Δv = ve ln m0 / m1 -gT.

 This gives, with gases at 2500 m / s about 600 kg of combustible materials to eject at 2500m / s. to slow down a 6000 kg machine

 Factors to consider:

-The details of the moment of ignition

-The direction of the jet of the retrorocket exactly in the direction of the race of the satellite.

 To stabilize a vessel in airless space, the only way is to react. It is necessary to act small rockets throwing their gas in the direction of the gyratory movements.

The mechanism of stabilization will consist of a set of small rockets arranged around the vessel and able to take action each in isolation in a given direction, according to the direction of the spinning and with the necessary force.

It is a gyroscopic system, with 3 degrees of freedom, which will guide the ship in space.

The ship will enter the atmosphere at a speed greater than 7km / s (25000 km / h). This will have 2 consequences:

 

- slowing down of the machine

- heating of the vessel by impact effect.

 

At this speed, the energy to be developed is enormous both in kinetic form due to speed and in potential form due to altitude.

 

The ideal would be a powerful braking (thus very consumer) before the arrival in the layers of the atmosphere then a vertical descent under parachute, but too energy consuming. We will use the drag of the machine in the atmosphere to slow it down. But we'll have to protect the ship from the heat.

 

There are two major classes of solutions. In the first this function is performed by an insulator placed under the surface material. In the second, it is the surface material itself.

 

Large orbiter-like returning objects of the space shuttle are subject to relatively modest environmental conditions, at least when compared to that of the space probes. Indeed the need to obtain low accelerations for human flight is accompanied by obtaining moderate heat flux. Hence the design of manoeuvering objects capable of large incidences at high altitude and thus a significant braking in the low-density slices of the atmosphere.

Reusable thermal protection

To obtain this result, the thermal operation is therefore based on the re-emission of a large part of the incident energy, obtained by a surface of high emissivity and on a material of low thermal conductivity.protection thermique


There are three types of regions:

-The front tip and the leading edges of the wings that support the most severe environmental conditions. A carbon-carbon material having a density of 1,980 kg / m.sup.3 is used which is obtained by textile spinning of carbon fibers impregnated with carbon obtained by pyrolysis of polymers. It is protected from oxygen by a deposit of silicon carbide. These pieces have a structural function. The maximum temperature is 1,900 K.

-The lower wind portion at the entrance consists of high-temperature Reusable Surface Insulation (HRSI) tiles comprising a structure formed of porous silica fibers (porosity 94%) surmounted by a borosilicate layer comprising an additive intended for increase the emissivity of the surface, hence its black appearance. The density is 140 kg / m3. The surface temperature is about 1,500 K.

-Least exposed parts are protected by Low-temperature Reusable Surface Insulation (LRSI) tiles similar to HRSI but with an aluminum oxide deposit that gives it a white color. They are qualified for use up to 900 K. They also participate in the thermal regulation in orbit, it is for this reason that one has chosen a surface having a high reflectivity thus a low emissivity.

Other insulators of lower performance are used locally. In total the thermal protection represents 10% of the total mass of the orbiter.

 

Given the complexity of the outer surface of a shuttle the thermal protection is cut into a large number of tiles (20 548 tiles on the space shuttle, 38 600 on Buran2). This leads to a complex technical management but also to an important problem constituted by the junction between two tiles. It is indeed necessary to reconcile the expansion with that of the entry of the hot gases in the interstice between two tiles.

Ablative systems

ex PICA Thermal Shield from the Mars Science Laboratory.

The heat shields used for space probes undergo a much more severe environment than that of the space shuttle. The maximum heat flux is in MW / m2: 5 for Apollo 4, 11 for Stardust, the most severe landfall ever made and up to 350 for Galileo

The actual value depends on the material through the parietal temperature and the phenomenon of injection of gases from physical or chemical decomposition and will oppose the convection of hot gases in the boundary layer.

This phenomenon reduces the heat flow but also the transfer of gases to the wall, in particular that of oxygen when it is presentboucler

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