The Rosetta mission orbiter Science overview the comet phase

TL;DR

The Rosetta mission orbiter provided comprehensive remote sensing and in situ analysis of comet 67P, revealing its composition, activity, and evolution, and offering insights into the origins of the solar system.

Contribution

This paper offers the first detailed overview of the Rosetta orbiter's operations and scientific findings during its comet phase from 2014 to 2016.

Findings

Mapped the comet's surface and environment

Analyzed the chemical and mineralogical composition

Studied the development of cometary activity

Abstract

The International Rosetta Mission was launched in 2004 and consists of the orbiter spacecraft Rosetta and the lander Philae. The aim of the mission is to map the comet 67P Churyumov Gerasimenko by remote sensing, to examine its environment insitu and its evolution in the inner solar system.Rosetta was the first spacecraft to rendezvous and orbit a comet, accompanying it as it passes through the inner solar system, and to deploy a lander, Philae and perform in situ science on the comet surface. The primary goals of the mission were to: characterize the comets nucleus; examine the chemical, mineralogical and isotopic composition of volatiles and refractories; examine the physical properties and interrelation of volatiles and refractories in a cometary nucleus; study the development of cometary activity and the processes in the surface layer of the nucleus and in the coma; detail the origin of comets, the relationship between cometary and interstellar material and the implications for the origin of the solar system; characterize asteroids, 2867 Steins and 21 Lutetia. This paper presents a summary of mission operations and science, focusing on the Rosetta orbiter component of the mission during its comet phase, from early 2014 up to September 2016.