SEARCHING FOR PLANET NINE WITH COADDED WISE AND NEOWISE-REACTIVATION IMAGES
- Berkeley Center for Cosmological Physics, Berkeley, CA 94720 (United States)
- Department of Physics and Astronomy, University of Utah, Salt Lake City, UT, 84112 (United States)
- Lawrence Berkeley National Laboratory, Berkeley, CA, 94720 (United States)
- Smithsonian Astrophysical Observatory, 60 Garden Street, Cambridge, MA 02138 (United States)
A distant, as yet unseen ninth planet has been invoked to explain various observations of the outer solar system. While such a “Planet Nine,” if it exists, is most likely to be discovered via reflected light in the optical, it may emit much more strongly at 3−5 μm than simple blackbody predictions would suggest, depending on its atmospheric properties. As a result, Planet Nine may be detectable at 3.4 μm with the Wide-field Infrared Survey Explorer, but single exposures are too shallow except at relatively small distances (d{sub 9}≲430 au). We develop a method to search for Planet Nine far beyond the W1 single-exposure sensitivity, to distances as large as 800 au, using inertial coadds of W1 exposures binned into ∼1 day intervals. We apply our methodology to a ∼2000 square degree testbed sky region which overlaps a southern segment of Planet Nine’s anticipated orbital path. We do not detect a plausible Planet Nine candidate, but are able to derive a detailed completeness curve, ruling out its presence within the parameter space searched at W1 < 16.66 (90% completeness). Our method uses all publicly available W1 imaging, spanning 2010 January to 2015 December, and will become more sensitive with future NEOWISE-Reactivation releases of additional W1 exposures. We anticipate that our method will be applicable to the entire high Galactic latitude sky, and we will extend our search to that full footprint in the near future.
- OSTI ID:
- 22863140
- Journal Information:
- The Astronomical Journal (Online), Vol. 153, Issue 2; Other Information: Country of input: International Atomic Energy Agency (IAEA); ISSN 1538-3881
- Country of Publication:
- United States
- Language:
- English
A new physical interpretation of optical and infrared variability in quasars
|
journal | July 2018 |
A 3 π Search for Planet Nine at 3.4 μ m with WISE and NEOWISE
|
journal | March 2018 |
Io’s Atmosphere Silhouetted by Jupiter Ly α
|
journal | September 2019 |
The exoplanet handbook: Book Review
|
journal | March 2012 |
A new physical interpretation of optical and infrared variability in quasars | text | January 2018 |
Similar Records
A 3$π$ Search for Planet Nine at 3.4 $μ$m with WISE and NEOWISE
A 3π Search for Planet Nine at 3.4 μm with WISE and NEOWISE