spinner
x
This website is using cookies, in order to track this cookie warning and other popups, for managing login sessions, and for website analytics. We do not collect or store personally identifiable information, nor track or display advertising related information. That's Fine
 - Galactic Exploration Catalog - 
Original submission for G2 Dust Cloud

Original submission, by CMDR Marx [2022-05-01 13:46:43]
DISCOVERER
NAME
G2 Dust Cloud
SYSTEMNAME
G2 Dust Cloud Sector JH-V c2-2851
CATEGORY
Stellar Features
CATEGORY 2
REGION
Galactic Centre
LATITUDE
LONGITUDE
CALLSIGN
SUMMARY
A faint cloud that has survived an encounter with Sagittarius A*.
DESCRIPTION

The G2 Dust Cloud is the remnant of an event observed in the 21st century, during which what was then suspected to be a gas cloud encountered Sagittarius A*. Since the event actually happened 26,000 years ago, by today the cloud has travelled quite a distance away from the centre. Explorers who visit it will find that it resembles a small and faint nebula, which can be observed by the naked eye only from within 80 ly. However, from up close, the cloud colours the bright light of the galactic core crimson red, which can make for some unique sights.

JOURNAL
OBSERVATORY
All content is licensed under Creative Commons (CC BY‑NC‑SA 3.0)

This website is not an official tool for the game Elite: Dangerous and is not affiliated with Frontier Developments. All information provided is based on publicly available information and data supplied by players, and may not be entirely accurate. 'Elite', the Elite logo, the Elite: Dangerous logo, 'Frontier' and the Frontier logo are registered trademarks of Frontier Developments plc. All rights reserved. All other trademarks and copyrights are acknowledged as the property of their respective owners.

Special thanks go to all commanders and explorers who graciously upload their data to EDDN, EDSM, and EDAstro to make all of this possible. We wouldn't exist without your data contributions. For any bug reports or feature suggestions, please visit our forum thread.