Over the past two decades NASA spacecraft missions obtained photographs permitting accurate size measurements of the planets and moons, and their surface features. Planetary global views are displayed at the same scale, in each picture to allow visual size comparisons. Additionally, special geographical features on some of the planets are compared

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The authors discuss two aspects related to the radial dependence of spatial density of interplanetary dust. First, they ask which spatial distribution the dust source should have to lead to the observed relative spatial distribution. Sources limited to a shell at several AU heliocentric distance are found to be inadequate, while extended (0.1 AU ≤

An analysis of 28 contiguous days of whole disk observations of the solar surface by means of optical resonant scattering in the K 769.9 nm line, taken at the Teide Observatory at Izana during July-August 1980, have thus far yielded two significant facts. Firstly when the results of an iterative sine-wave fitting procedure are considered in the

OVINAS CON SUS DIFERENTES CONNOTACIONES. OTRO ASPECTO ESTUDIADO FUE LA SUPERVIVENCIA DE LAS L-I TANTO EN CONDICIONES CONTROLADAS COMO NATURALES. Y POR ULTIMO LA EVOLUCION EN EL INTERMEDIARIO CON DIFERENTE NUMERO DE LARVAS Y LA PRESENCIA DE ESTAS EN MOLUSCOS PROCEDENTES DE ZONAS QUE SE SABIAN CONTAMINADAS COMO CONDICIONANTES DE FUTURAS INFESTACIONES

SE HAN ESTUDIADO VARIOS ASPECTOS DE LA EMERGENCIA DE LAS REGIONES ACTIVAS (RA) EN EL SOL A FIN DE CLARIFICAR LAS PROFUNDAS DIFERENCIAS EXISTENTES ENTRE RA GRANDES (DIAMETRO 510 ELEVADO A 21MX) Y PEQUEÑAS. EN UN ESTUDIO ESTADISTICO SE OBSERVA QUE UNA CONDICION NECESARIA PARA LA EMERGENCIA DE RA PEQUEÑAS ES LA EXISTENCIA DE RESTOS MAGNETICOS DE UNA