4.6 Article

OBSERVATION OF TWO NEW L4 NEPTUNE TROJANS IN THE DARK ENERGY SURVEY SUPERNOVA FIELDS

Journal

ASTRONOMICAL JOURNAL
Volume 151, Issue 2, Pages -

Publisher

IOP PUBLISHING LTD
DOI: 10.3847/0004-6256/151/2/39

Keywords

minor planets, asteroids: general

Funding

  1. U.S. Department of Energy
  2. U.S. National Science Foundation
  3. Ministry of Science and Education of Spain
  4. Science and Technology Facilities Council of the United Kingdom
  5. Higher Education Funding Council for England
  6. National Center for Supercomputing Applications at the University of Illinois at Urbana-Champaign
  7. Kavli Institute of Cosmological Physics at the University of Chicago
  8. Financiadora de Estudos e Projetos
  9. Fundacao Carlos Chagas Filho de Amparo a Pesquisa do Estado do Rio de Janeiro
  10. Conselho Nacional de Desenvolvimento Cientifico e Tecnologico
  11. Ministerio da Ciencia e Tecnologia
  12. Deutsche Forschungsgemeinschaft
  13. Argonne National Laboratory
  14. University of California at Santa Cruz
  15. University of Cambridge
  16. Centro de Investigaciones Energeticas
  17. Medioambientales y Tecnologicas-Madrid
  18. University of Chicago
  19. University College London
  20. DES-Brazil Consortium
  21. Eidgenossische Technische Hochschule (ETH) Zurich
  22. Fermi National Accelerator Laboratory
  23. University of Edinburgh
  24. University of Illinois at Urbana-Champaign
  25. Institut de Ciencies de l'Espai (IEEC/CSIC)
  26. Institut de Fisica d'Altes Energies
  27. Lawrence Berkeley National Laboratory
  28. Ludwig-Maximilians Universitat
  29. associated Excellence Cluster universe
  30. University of Michigan
  31. National Optical Astronomy Observatory
  32. University of Nottingham
  33. Ohio State University
  34. University of Pennsylvania
  35. University of Portsmouth
  36. SLAC National Accelerator Laboratory
  37. Stanford University
  38. University of Sussex
  39. Texas AM University
  40. Science and Technology Facilities Council [ST/K00090X/1, ST/M001334/1] Funding Source: researchfish
  41. STFC [ST/M003574/1, ST/H001581/1, ST/L000652/1, ST/K00090X/1, ST/M001334/1, ST/N001087/1, ST/L006529/1, ST/I000976/1] Funding Source: UKRI
  42. Division Of Astronomical Sciences
  43. Direct For Mathematical & Physical Scien [1515015, 1311924] Funding Source: National Science Foundation
  44. Division Of Physics
  45. Direct For Mathematical & Physical Scien [GRANTS:13530420, 1262543] Funding Source: National Science Foundation
  46. Division Of Physics
  47. Direct For Mathematical & Physical Scien [1125897] Funding Source: National Science Foundation
  48. ICREA Funding Source: Custom

Ask authors/readers for more resources

We report the discovery of the eighth and ninth known Trojans in stable orbits around Neptune's leading Lagrange point, L4. The objects 2014. QO(441) and 2014. QP(441) were detected in data obtained during the 2013-14 and 2014-15 observing seasons by the Dark Energy Survey, using the Dark Energy Camera (DECam) on the 4-m Blanco telescope at Cerro Tololo Inter-American Observatory. Both are in high-inclination orbits (18 degrees.8 and 19 degrees.4, respectively). With an eccentricity of 0.104, 2014. QO(441) has the most eccentric orbit of the 11 known stable Neptune Trojans. Here we describe the search procedure and investigate the objects' long-term dynamical stability and physical properties.

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