skip to main content
US FlagAn official website of the United States government
dot gov icon
Official websites use .gov
A .gov website belongs to an official government organization in the United States.
https lock icon
Secure .gov websites use HTTPS
A lock ( lock ) or https:// means you've safely connected to the .gov website. Share sensitive information only on official, secure websites.


Title: Discovery of Dust Emission Activity Emanating from Main-belt Asteroid 2015 FW412
Abstract We present the discovery of activity emanating from main-belt asteroid 2015 FW412, a finding stemming from the Citizen Science projectActive Asteroids, a NASA Partner program. We identified a pronounced tail originating from 2015 FW412and oriented in the anti-motion direction in archival Blanco 4 m (Cerro Tololo Inter-American Observatory, Chile) Dark Energy Camera images from UT 2015 April 13, 18, 19, 21 and 22. Activity occurred near perihelion, consistent with the main-belt comets (MBCs), an active asteroid subset known for sublimation-driven activity in the main asteroid belt; thus 2015 FW412is a candidate MBC. We did not detect activity on UT 2021 December 12 using the Inamori-Magellan Areal Camera and Spectrograph on the 6.5 m Baade telescope, when 2015 FW412was near aphelion.  more » « less
Award ID(s):
1950901
PAR ID:
10610710
Author(s) / Creator(s):
; ; ; ; ; ; ; ;
Publisher / Repository:
IOP
Date Published:
Journal Name:
Research Notes of the AAS
Volume:
7
Issue:
2
ISSN:
2515-5172
Page Range / eLocation ID:
22
Format(s):
Medium: X
Sponsoring Org:
National Science Foundation
More Like this
  1. Abstract We announce the discovery of activity, in the form of a distinct cometary tail, emerging from main-belt asteroid 2015 VA108. Activity was first identified by volunteers of the Citizen Science project Active Asteroids (a NASA Partner). We uncovered one additional image from the same observing run which also unambiguously shows 2015 VA108with a tail oriented between the anti-solar and anti-motion vectors that are often correlated with activity orientation on sky. Both publicly available archival images were originally acquired UT 2015 October 11 with the Dark Energy Camera (DECam) on the Blanco 4 m telescope at the Cerro Tololo Inter-American Observatory (Chile) as part of the Dark Energy Camera Legacy Survey. Activity occurred near perihelion and, combined with its residence in the main asteroid belt, 2015 VA108is a candidate main-belt comet, an active asteroid subset known for volatile sublimation. 
    more » « less
  2. Abstract We report the discovery of cometary activity emanating from Main-belt asteroid 410590 (2008 GB140), a finding facilitated, for the first time, by an artificial intelligence (AI) assistant. The assistant,TailNet, is a prototype we designed to enhance volunteer efforts of our Citizen Science projectActive Asteroids, a NASA Partner program hosted on theZooniverseplatform. Our follow-up investigation revealed eight Dark Energy Camera images showing 2008 GB140with a tail spanning UT 2023 April 23–UT 2023 July 3, when the object was inbound to perihelion. We classify 2008 GB140as an active asteroid and a candidate Main-belt comet (MBC)—a main-belt asteroid that undergoes volatile sublimation-driven activity. Notably, 2008 GB140is presently near perihelion, thus the object is a prime target for follow-up observations to further characterize its activity. 
    more » « less
  3. Abstract We report the discovery of an active asteroid, 2016 UU121, for the first time via artificial intelligence-enhanced classification, informed by our NASA Partner programActive Asteroids, a Citizen Science project hosted on theZooniverseplatform. The early version of our deep neural network,TailNet, identified potential activity associated with 2016 UU121in 40 Dark Energy Camera (DECam) images from UT 2021 September 10 to 11. The discovery was vetted and confirmed by ourActive Asteroidscore science team. In total, 66 DECam images of this object showed clear activity in the form of a tail. 2016 UU121has a Tisserand parameter with respect to Jupiter of 3.161, thus we classify the object as an active asteroid. Moreover, the activity occurred near perihelion, so 2016 UU121is also a candidate Main-belt comet. 
    more » « less
  4. Abstract We present evidence that, on UT 2018 February 15, main-belt asteroid (588045) 2007 FZ18displayed cometary activity in the form of two tails, one each in the anti-solar and anti-motion directions. Activity was first identified by volunteers of the NASA Partner program Active Asteroids, a Citizen Science program hosted on the Zooniverse platform, in an image acquired with the Dark Energy Camera on the Blanco 4 m telescope at the Cerro Tololo Inter-American Observatory in Chile. Notably, (588045) 2007 FZ18is inbound toward perihelion, so telescope observations are timely to detect a possible second activity outburst. 
    more » « less
  5. Abstract We report that minor planet 2004 CV50displayed cometary activity in the form of a short, diffuse tail, first identified by volunteers of the Citizen Science programActive Asteroids, a NASA Partner program hosted on theZooniverseonline platform. The activity is present in three images, from UT 2020 February 15 and UT 2020 March 14, that were acquired with the Dark Energy Camera on the Blanco 4 m telescope at the Cerro-Tololo Inter-American Observatory in Chile. We find that 2004 CV50is most likely an active quasi-Hilda object rather than an active asteroid, despite 2004 CV50having a Tisserand parameter with respect to Jupiter of 3.06. 
    more » « less