Future Space Missions with Bernese Involvement

The University of Bern is not only contributing to missions already launched, researchers and engineers from CSH and WP are also currently engaged in the development of instruments intended for future missions.

This page is currently under construction, more information will be available soon.

2028 | Asteroid Apophis | ESA and JAXA Mission

RAMSES — CHANCES Camera

More information will be available soon.

2028/2029 | Comets | ESA and JAXA Mission

© ESA

Comet Interceptor — CoCa Camera & Mass Analyzer MANiaC

Comet Interceptor will be the first mission to visit a comet coming directly from the outer reaches of the Sun's realm, carrying material untouched since the dawn of the Solar System. The joint ESA-JAXA mission combines the breakthroughs in comet discoveries from Giotto and Rosetta with a compact, agile set of spacecraft that can intercept and study long period comets entering the inner Solar System for the first time or possibly other interstellar objects. After launch, the mission will be "parked" in space where it awaits the arrival of a suitable pristine comet. Among the instrument suite are the Comet Camera (CoCa) and the Mass Analyzer for Neutrals in a Coma (MANiaC), which are being developed at the University of Bern. CoCa will obtain high resolution images of the comet's nucleus while MANiaC will sample the released gases.

Following the Call for Missions in July 2018, the F-Class mission Comet Interceptor was selected by ESA on June 19, 2019. Upon completion of an initial study phase, the mission was formally adopted and approved for construction by ESA on June 08, 2022.

Comet Interceptor is set to launch in late 2028 or early 2029 alongside the ESA mission Ariel from Europe's Spaceport in French Guiana. Analysis of the first measurements is expected in the 2030s, as soon as a first comet encounter has occured.

CoCa

The Comet Comera (CoCa) is the imaging system on Comet Interceptor's primary spacecraft and is provided by a consortium led by the University of Bern. It is designed to provide high resolution imaging of the nucleus of the selected comet in four filters at selected broadband optical wavelengths. CoCa is based on the stereographic camera Colour and Stereo Surface Imaging System (CaSSIS) on the ExoMars Trace Gas Orbiter mission to Mars, which was also developed at the University of Bern. The system is constructed to provide over 2500 images during the fly-by and can allow saturation on the nucleus to provide optimum signal-to-noise on the dust coma at all times through the fly-by.

MANiaC

The Mass Analyzer for Neutrals in a Coma (MANiaC) instrument, also located on the primary spacecraft, is made up of a time-of-flight mass spectrometer and a neutral density gauge, both attached to an electronics unit. The combination of the two sensors enables measurements of the absolute neutral gas densitites of different volatile species along the fly-by trajectory of the Comet Interceptor spacecraft. MANiaC is set to measure the abundances of the major volatile species in the cometary coma (atoms, molecules and small ice particles), their mass and chemical make-up, and may also be able to measure minor species such as organic molecules and optain information on the composition of dust grains.