Related Experiment Video
Updated: Aug 8, 2025

Method for Recording Broadband High Resolution Emission Spectra of Laboratory Lightning Arcs
Published on: August 27, 2019
Light curves and colours of the ejecta from Dimorphos after the DART impact
Ariel Graykowski1, Ryan A Lambert2, Franck Marchis2,3
1SETI Institute, Carl Sagan Center, Mountain View, CA, USA. agraykowski@seti.org.
Abstract:
On 26 September 2022, the Double Asteroid Redirection Test (DART) spacecraft struck Dimorphos, a satellite of the asteroid 65803 Didymos1. Because it is a binary system, it is possible to determine how much the orbit of the satellite changed, as part of a test of what is necessary to deflect an asteroid that might threaten Earth with an impact. In nominal cases, pre-impact predictions of the orbital period reduction ranged from roughly 8.8 to 17 min (refs. 2,3). Here we report optical observations of Dimorphos before, during and after the impact, from a network of citizen scientists' telescopes across the world. We find a maximum brightening of 2.29 ± 0.14 mag on impact. Didymos fades back to its pre-impact brightness over the course of 23.7 ± 0.7 days. We estimate lower limits on the mass contained in the ejecta, which was 0.3-0.5% Dimorphos's mass depending on the dust size. We also observe a reddening of the ejecta on impact.
Related Concept Videos
Flame Photometry: Overview
Emission Spectra
Flame Photometry: Lab
Atomic Emission Spectroscopy: Overview
Interaction of EM Radiation with Matter: Spectroscopy
Doppler Effect - II

