Data from NASA's Wide-field Infrared Survey Explorer, or WISE, has found no evidence for a hypothesized body sometimes referred to as "Planet X." This body was thought to be a large planet or small star orbiting in the far reaches of our solar system. Astronomers searched millions of images taken by WISE over the whole sky, finding no Saturn-like body out to a distance of 10,000 astronomical units (au) from the sun, and no Jupiter-like body out to 26,000 au. One astronomical unit equals 93 million miles. Earth is 1 au, and Pluto about 40 au, from the sun.
This chart shows what types of objects WISE can and cannot see at certain distances from our sun. Bodies with larger masses are brighter, and therefore can be seen at greater distances. For example, if a Jupiter-mass planet existed at 10,000 au, WISE would have easily seen it. But WISE would not have been able to see a Jupiter-mass planet residing at 100,000 au -- it would have been too faint.
The chart was created by Janella Williams of Penn State University, University Park, Pa.
WISE was put into hibernation upon completing its primary mission in 2011. In September 2013, it was reactivated, renamed NEOWISE and assigned a new mission to assist NASA's efforts to identify the population of potentially hazardous near-Earth objects. NEOWISE will also characterize previously known asteroids and comets to better understand their sizes and compositions.
More information is online at http://www.nasa.gov/wise and http://wise.astro.ucla.edu and http://www.jpl.nasa.gov/wise .
Name | Value | Additional Values |
---|---|---|
Target | ||
System | Kuiper Belt | |
Target Type | Dwarf Planet | KBO |
Mission | Near-Earth Object Wide-field Infrared Survey Explorer (NEOWISE) | |
Instrument Host | NEOWISE | |
Host Type | Space Telescope | |
Instrument | ||
Detector | ||
Extra Keywords | Color, Infrared | |
Acquisition Date | ||
Release Date | 2014-03-07 | |
Date in Caption | ||
Image Credit | Penn State University | |
Source | photojournal.jpl.nasa.gov/catalog/PIA17990 | |
Identifier | PIA17990 |