Skip to main content
Skip to navigation
Skip to footer
DLR Portal
Press
Accessibility
de
en
Institute of
Planetary Research
About us
About us
▾
The Institute of Planetary Research
▾
Departments
▾
Planetary Physics
▾
Planetary Geology
▾
Planetary Geodesy
▾
Extrasolar Planets and Atmospheres
▾
Planetary Sensor Systems
▾
Planetary Laboratories
▾
Central Institute Infrastructure
▾
Location & getting there
Research & Transfer
Research & Transfer
▾
Research Topics
▾
Planets and Moons in the Solar System
▾
Small Bodies (Asteroids and Comets)
▾
Extrasolar Planets and Planetary Systems
▾
Habitability and Biosignatures
▾
Missions and Projects
▾
BepiColombo
▾
BioSigN
▾
CHEOPS
▾
Comet Interceptor
▾
EnVision
▾
Hayabusa2/Hayabusa2#
▾
Hera
▾
JUICE
▾
Lucy
▾
Mars 2020 and ExoMars
▾
Mars Express
▾
MMX
▾
PLATO
▾
Psyche
▾
VERITAS
▾
Finished Missions
▾
Research Infrastructure
▾
Assembly, Integration and Verification (AIV)/Laser Laboratory
▾
Calibration and Thermal Vacuum Laboratory
▾
Sensor Design and Test Laboratory
▾
Detector Characterisation Laboratory (DCL)
▾
Planetary Spectroscopy Laboratory
▾
Sample Preparation Laboratory
▾
Mars Simulation Facility
▾
Planetary Simulation Laboratory
▾
Raman Mineral- and Bio-Detection Laboratory
▾
Thermal Laboratory
▾
Cooperation opportunities
▾
National universities
▾
National research institutions
▾
National industrial companies
▾
International cooperations
▾
Networks
▾
Publications (elib)
Latest
Latest
▾
News
▾
Events
▾
FAQ
▾
How can I recognise a meteorite?
Media
Media
▾
Regional Planetary Image Facility (RPIF)
Careers & Education
Careers & Education
▾
Vacancies
▾
Information for students
>
Media
>
Images
>
Other Images
>
>
FAQ
>
No meteorites
Home
>
Media
>
Images
>
Other Images
>
FAQ
>
No meteorites
No meteorites
No meteorites
These stones are not meteorites. From top left to bottom right: Pyrite nodule, vesicular slag, limonite concretion, Marcasite nodule, glassy slag.
Credit:
Dieter Heinlein
