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handle: 10261/29517
A pesar de que el arco recorrido sobrepasa ya los 300", los elernentos de este par, período, excentricidad y semieje mayor, son todavía inciertos debido a que el apastro aún no ha sido alcanzado y en el periastro las observaciones, aunque numerosas, son todas ilusorias.
Publicado en "Vrania", núm. 237.
Peer reviewed
Astronomía, Órbitas, Estrellas
Astronomía, Órbitas, Estrellas
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