Universal Astrobiology on the Solar System Dwarf Planet Ceres: A Review

Abstract

As the solar spacecraft closes in for its orbital popularity above Vesta at a safe mode altitude of approximately four hundred kilometers above Vesta's surface there exists two in all likelihood smaller asteroid satellites showed by using a HST picture taken of Vesta in 2006.These asteroids are demonstrated a second time in one of the photographs taken by using the dawn Spacecraft onboard cameras on July 09th, 2011. Every asteroid measures one and half of a kilometer to at least one - kilometer in length. But, the question is; it viable that these smaller asteroids ought to have posed a risk to the sunrise spacecraft? In that case, is it additionally feasible that other moon-like satellites ought to pose a difficulty for the sunrise Spacecraft while it makes its way to Ceres, wherein it can arrive sometime in the course of the summer of 2015? This paper proposes to answer this and different questions on this subject as nicely. But, these asteroids had been found using a brand new space exploration imaging era known as IMMI. That is the acronym for - (limitless - Microscopic –Macroscopic Imaging)? (See important footnote under). Wherein the dawn Spacecraft did now not look at nor was there preceding expertise of its lifestyles. Consequently, this paper is to make the clinical network conscious in both astronomy and astrophysics privy to what changed into no longer acknowledged when Vesta turned into investigated via the dawn Spacecraft and what it ought to additionally be aware of on it's the manner to Ceresin like manner.

Keywords: Ceres, Dwarf planets, solar system, Panspermia, Fred Hoyle