New Neliota project detects flashes from lunar impacts

New Neliota project detects flashes from lunar impacts
Since March 2017, the NELIOTA project has been monitoring the dark side of the Moon for flashes of light caused by tiny pieces of rock striking the moon's surface. Credit: NELIOTA project

Using a system developed under an ESA contract, the Greek NELIOTA project has begun to detect flashes of light caused by small pieces of rock striking the moon's surface. NELIOTA is the first system that can determine the temperature of these impact flashes.

Studies such as NELIOTA are important because Earth and its moon are constantly bombarded by natural space debris. Most of this material ranges in size from dust particles to small pebbles, although larger objects can appear, unexpectedly, from time to time. This was the case when an object almost 20 m in diameter disintegrated above the Russian city of Chelyabinsk in February 2013. The resultant explosion, caught on camera, caused considerable damage, although, fortunately, no one was killed.

Particles only millimetres across usually appear several times per hour on any clear dark night in the form of meteors or 'shooting stars'. However, the number of incoming objects in the size range from decimetres to metres is not well known. Too small to be detected directly with telescopes, they are rarely captured by cameras when they enter Earth's atmosphere.

One way to determine the number of larger impactors and the potential impact threat to Earth is to observe the moon, in particular the dark area not illuminated by the Sun. When small asteroids strike the lunar surface at high speed, they burn up on impact, generating a brief flash of light, which can be visible from Earth. Assuming a typical velocity and density, the size and mass of the object can be estimated from the brightness of the event.

A new campaign to study these lunar flashes is being undertaken by the NELIOTA (Near-Earth object Lunar Impacts and Optical TrAnsients) project, which began operation on 8 March 2017. NELIOTA utilises a refurbished telescope, which is operated by the National Observatory of Athens and located close to the Greek town of Kryoneri.

New Neliota project detects flashes from lunar impacts
Since March 2017, the refurbished 1.2m Kryoneri telescope near the Greek town of Kryoneri has been used for the NELIOTA project. Credit: Theofanis Matsopoulos

The 1.2 m telescope splits incoming light into two colours and uses two advanced digital cameras to record the data at a rate of 30 frames per second. Observations of the moon's night hemisphere are made whenever Earth's natural satellite is above the horizon and mainly dark – between New moon and the first quarter phase, or between last quarter and New moon.

Automated software analyses the video obtained and identifies possible impact flashes. Camera effects can be excluded by identifying events that are only visible in both cameras. The cameras operate in different colour ranges, allowing the temperature of the impact flash to be estimated – NELIOTA is the first system of this type to have the potential to determine the temperature of these flashes.

The exceptional capability of the telescope was confirmed during its pre-operational, commissioning phase, when it recorded four impact flashes in about 11 hours of observing time. The task is now to observe these flashes on the dark side of the moon over a period of 22 months.

"Its large telescope aperture enables NELIOTA to detect fainter flashes than other lunar monitoring surveys and provides precise colour information not currently available from other projects," says Alceste Bonanos, the Principal Investigator for NELIOTA.

"Our twin camera system allows us to confirm lunar impact events with a single telescope, something that has not been done before. Once data have been collected over the 22-month long operational period, we will be able to better constrain the number of NEOs (near-Earth objects) in the decimetre to metre size range.

New Neliota project detects flashes from lunar impacts
Since March 2017, the NELIOTA project has been monitoring the dark side of the Moon for flashes of light caused by tiny pieces of rock striking the moon's surface. Credit: NELIOTA project
"The data will also help to determine the physics of impact flashes. We are analysing the flashes in collaboration with the Science Support Office of ESA, in order to measure the temperature of each and estimate the mass, size of the impactor and crater size created from the ."

"These observations are very relevant for our Space Situational Awareness programme. In particular, in the size range we can observe here, the number of objects is not very well known. Performing these observations over a longer period of time will help us to better understand this number," says Detlef Koschny, co-manager of the near-Earth object segment in ESA's Space Situational Awareness programme, and a scientist in the Science Support Office.

NELIOTA is also contributing to public outreach and education.

"We are currently training two PhD students to operate the Kryoneri telescope and conduct lunar monitoring observations," says Alceste.

"We also organise public tours of Kryoneri Observatory, during which we present the NELIOTA project, as well as talks on near-Earth asteroids for students and for the general public. This year, we plan to participate in Asteroid Day 2017, by organising a public event at Kryoneri Observatory on 30 June."

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Citation: New Neliota project detects flashes from lunar impacts (2017, May 25) retrieved 16 June 2019 from
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User comments

May 25, 2017
The observed flashes are most likely from electrical discharge, not impact. The fine lunar surface dust is from the disintegration of any object, small or large, when it gets close enough to the surface. Even the largest craters are from a discharge event, but without functioning seismic sensors on the Moon, this can not be confirmed. The sensors on the Moon delivered by the Apollo crews found the Moon to be seismically silent. a discharge is not going to produce an impact type shock.

Lunar electric fields, surface potential and associated plasma sheaths

May 26, 2017
The seismographs carried by Apollo were not sensitive enough to pick up the impact of a meter-sized object more than a kilometer away. They were designed to listen for crustal movements and magma, since that was the only type of seismic detection that they knew how to do at the time.

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