Solar sailing is considered one of the most promising propulsion systems for interplanetary missions, and an efficient way to conduct orbital manoeuvre. The solar pressure acts on a large membrane that produces the propellant-less thrust. The solar sail is made of lightweight-reactive materials generally fabricated by polyimides with a one-side aluminium coating. The sail dimensions are conventionally huge in order to provide the proper thrust. In this work, we propose to eliminate the aluminium coating and to realize the membrane only by using polyimides. In particular, we analyse the propulsion performances of inexpensive polyimide membranes, such as Kapton HN and Kapton B. The selected polyimides films present different optical behaviour due to their different sunlight reactance: Kapton HN is semi-transparent, whereas Kapton B is black pigmented. We perform experimental measurements to determine the optical parameters of both films. These parameters are then used to determine the thrust of the two membranes. The solar sail that we investigate has a square geometry with dimensions of 6 m X 6 m and in thickness. The characteristic acceleration is the same for both membranes and equal to 0.01 mm/s2. Kapton HN produces a greater thrust than Kapton B, even if Kapton B exhibits a highest emissivity. These results can be explained highlighting the be-reactive nature of the selected thin films. In order to take advantage from the high emissivity of Kapton B and enhancing the thrust modulus, we consider modifying the surface roughness of one side of the membrane. In this way, the propulsion performance can be improved by exploiting the difference of roughness between the membrane sides. Orbital simulation shows that the sail is able to maintain efficiently the station keeping in Halo orbit around the Lagrange point of the Sun-Earth system.
Solar sail: a comparative study between Kapton HN and Kapton B membranes / Laurenzi, Susanna; S., Pizzurro; Circi, Christian. - ELETTRONICO. - 9:(2014), pp. 6161-6166. (Intervento presentato al convegno 65th International Astronautical Congress 2014: Our World Needs Space, IAC 2014 tenutosi a Toronto, Canada nel 29 September – 3 October, 2014).
Solar sail: a comparative study between Kapton HN and Kapton B membranes
LAURENZI, SUSANNA;CIRCI, Christian
2014
Abstract
Solar sailing is considered one of the most promising propulsion systems for interplanetary missions, and an efficient way to conduct orbital manoeuvre. The solar pressure acts on a large membrane that produces the propellant-less thrust. The solar sail is made of lightweight-reactive materials generally fabricated by polyimides with a one-side aluminium coating. The sail dimensions are conventionally huge in order to provide the proper thrust. In this work, we propose to eliminate the aluminium coating and to realize the membrane only by using polyimides. In particular, we analyse the propulsion performances of inexpensive polyimide membranes, such as Kapton HN and Kapton B. The selected polyimides films present different optical behaviour due to their different sunlight reactance: Kapton HN is semi-transparent, whereas Kapton B is black pigmented. We perform experimental measurements to determine the optical parameters of both films. These parameters are then used to determine the thrust of the two membranes. The solar sail that we investigate has a square geometry with dimensions of 6 m X 6 m and in thickness. The characteristic acceleration is the same for both membranes and equal to 0.01 mm/s2. Kapton HN produces a greater thrust than Kapton B, even if Kapton B exhibits a highest emissivity. These results can be explained highlighting the be-reactive nature of the selected thin films. In order to take advantage from the high emissivity of Kapton B and enhancing the thrust modulus, we consider modifying the surface roughness of one side of the membrane. In this way, the propulsion performance can be improved by exploiting the difference of roughness between the membrane sides. Orbital simulation shows that the sail is able to maintain efficiently the station keeping in Halo orbit around the Lagrange point of the Sun-Earth system.I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.