Satellite Cluster Research Articles

Technical and economical comparison between a modular geostationary space platform and a cluster of satellites

In recent years, the identification of a large number of telecommunication missions reflects a growing demand for the provision of a large variety of communications and data transmission services performed by a space segment. At present, communication space segment use a single operational satellite per orbit position. However, the expected increase of communication channels per space segment will lead to a corresponding increase of satellite mass and size which could exceed the capabilities of existing launch vehicles in terms of mass and volume requirements. Those considerations, coupled with the threatening saturation of the geostationary orbit, lead to the conclusion that an optimal space segment concept must be defined on a technical as well as economical point of view. Two main concepts may be envisaged: one is a large platform, which can be assembled either in geostationary orbit (resulting in several launches, rendez-vous and docking), or in low earth orbit by using the STS; the other concept is a cluster of satellites. These candidate concepts are designed to meet the requirements of a reference mission. They are characterized by the required number of modules to be launched, the type of launcher, the new subsystems or equipments to be developed. The concepts are evaluated following technical criteria such as adaptability to other missions, flexibility, growth potential. A cost/benefit evaluation of each solution is presented. A comparison between the different concepts is then made on the basis of the technical/economical attractiveness of each solution.

Multiple forms of vitamin D-dependent calcium-binding protein in rat kidney.

The technique of two-dimensional electrophoresis was used in combination with a highly sensitive silver stain to study vitamin D-dependent calcium-binding protein (CaBP) in rat kidney. Rat renal CaBP was shown to co-migrate almost exactly with CaBP purified from chick intestine suggesting evolutionary conservation of this protein. In some cases rat renal CaBP appeared not as a single polypeptide, but rather as a cluster of 4 polypeptides. Formation of the satellite cluster of CaBP in response to high doses of 1,25-dihydroxyvitamin D3 occurred in young rats which had been maintained on a vitamin D-deficient diet for 2 weeks, as well as in older rats which had been maintained on the same diet for 5 months. The 4 forms of CaBP were not the result of various states of Ca2+ binding, but rather the result of an enzymatic reaction. This was shown by 3 experiments. 1) Adding excess EGTA to samples containing the 4 satellite forms did not change the two-dimensional electrophoretogram. 2) Incubation of purified chick intestinal CaBP with kidney cytosols from D-deficient rats brought about the formation of the satellite CaBP forms from the chick protein. However, purified chick CaBP was unchanged by incubation in buffer alone for up to 2 h at 37 degrees C. 3) Placing rat kidney cytosols in a boiling water bath for 10 min inactivated the factor which generated the satellite forms as would be expected for an enzyme. The physiological significance of these forms of CaBP is as yet unknown.

Restriction enzyme banding of mouse metaphase chromosomes.

Fixed metaphase chromosomes from mouse strain RIII embryos or A9 cells were treated with a restriction endonuclease, followed by Giemsa staining. Alu I, Hinf I, or Mbo I treatment produced a C-band pattern, and Eco RII or Hae III produced a G-band plus C-band pattern. Ava II and Bst NI each produced a G-band pattern, but on most chromosomes only a small segment of each C-band, adjacent to the centromere, was stained. These tiny residual C-bands may contain a minor satellite located adjacent to the major satellite clusters.

Gas drag in primordial circumplanetary envelopes: A mechanism for satellite capture

Some natural satellites may have been captured due to the gas drag they experienced in passing through primordial circumplanetary nebulas. This paper models such an encounter and derives the testable parameters from the known properties of current solar system objects and Bodenheimer's (1977, Icarus 31) model of the earliest phases of Jupiter's evolution. We propose that the clusters of prograde and retrograde irregular satellites of Jupiter originated when two parent bodies were decelerated and fragmented as they passed through an extended primordial Jovian nebula. Fragmentation occured because the gas dynamic pressure exceeded the parent bodies' strengths. These events must have occurred only shortly before the primordial nebula experienced hydrodynamical collapse so that subsequently the fragments underwent only limited orbital evolution. Because self-gravity exceeded the relative drag force, the fragments initially remained together, only to be dispersed at a later time by a collision with a stray body. Predictions of this hypothesis, such as orbital distance of the irregular satellites and size of the parent bodies, are found to be consistent with the observed properties of Jupiter's irregular satellites. In addition nebular drag at a later time may have caused the inner three Galilean satellites to undergo a modest amount of orbital evolution, accounting for their present orbital resonance. Gas drag capture of Saturn's Phoebe and Iapetus and Neptune's Nereid and Triton may also be possible. Reasonable differences in properties could explain why these satellites, in contrast to the Jovian ones, did not fracture upon capture. The current irregular satellites represent only a tiny fraction of the bodies captured by primordial nebulas. The dominant fraction would have spiraled into the center of the nebula as a result of continued gas drag and thus offer one source for the heavy element cores of the outer planets. If one is willing to postulate the presence of a massive gaseous nebula around primordial Mars, then gas drag capture could account for the origin of the Martian moons. We hypothesize that a single parent body was captured in a region of the nebula where the gas velocity approached the Keplerian value, that it fragmented upon deceleration into at least two bodies, Phobos and Deimos, and that continued nebular drag led to the low eccentricity and inclination that characterize the satellites' current orbits. Following the dissipation of this nebula, the more massive Phobos tidally evolved to its current position.

Cluster Geometry Recovery For Colocated Satellites

Hill's equations of relative motion are applied to the problem of re-initialising the relative orbit of a cluster of Geosynchronous satellites which have deviated from their nominal relative orbits to such an extent that there exists an unacceptably high collision or telecommunication interference risk. A solution is presented for satellites possessing thruster capability along two perpendicular axes, the longitudinal direction and the latitudinal direction, which correspond to the burn directions used for East-West and North-South station keeping of GEO satellites.

Application of the multiple satellite concept to particles and fields research

Four satellite cluster laboratory in near-earth environment to investigate solar-terrestrial relationships, emphasizing interaction of solar wind and magnetosphere

Gold Satellite Clusters on Muscovite Mica

Groups of gold clusters consisting of a large main cluster and smaller satellite clusters within a few tens of angstroms of the main cluster are nucleated from vapor on the cleavage face of muscovite mica in ultra-high vacuum. The satellites are seen for low cluster nucleation densities for which the random occurrence of such close cluster formations is extremely unlikely. The dependence of the average frequency of satellite occurrence per cluster upon substrate temperature and gold flux is examined. In addition, the relationship between the frequency of satellite observation and the diameters of the clusters with satellites is studied for fixed evaporation conditions. The satellites are tentatively interpreted as resulting from cluster nucleation on gold atom pairs which have escaped from established parent clusters.