The solar system has eight planets. In 2006, astronomers reclassified Pluto as a dwarf planet, the same class that contains Eris, Sedna, Quaoar, Ceres and perhaps many more solar system small bodies. These are defined approximately as bodies that orbit the sun but that are not massive enough (unlike regular planets) to gravitationally dominate their environments by clearing away material. Astronomers wonder, though, whether there might not really be a ninth planet previously undiscovered but lurking in the outer reaches of the solar system, perhaps in the giant Oort cloud of objects that begins hundreds of astronomical units (au) from the sun and extends outward.
The notion that there may be a ninth massive planet in the outer solar system has taken on new appeal with recent data that show that the orbital parameters of some small bodies beyond Neptune (their inclinations, perihelions, and retrograde motions) seem to behave as though they had been influenced by the gravity of a massive object in the outer solar system. Although these data suffer from observational biases and statistical uncertainties, they have triggered renewed interest in the idea of the presence of another planet.
This speculative Planet 9, according to estimates, would be about 5 to 10 Earth masses in size and orbit about 400 to 800 au from the sun. A planet at this distance would be extremely difficult to spot in normal optical sky searches because of its faintness, even to telescopes like PanSTARRS and LSST. Most solar system objects were discovered at optical wavelengths via their reflected sunlight, but the sunlight they receive drops, as the inverse square law for electromagnetic radiation says that measured light intensity is inversely proportional to the distance squared from the source of radiation; moreover, the reflected portion then travels back to telescopes on Earth and so declines again by a similar factor.
The potential Planet 9 spectra compared to the 5σ detection limit of current and upcoming wide-area surveys. © The Astrophysical Journal (2021). DOI: 10.3847/1538-4357/ac2307
In the outer reaches of the solar system these objects, although cold, might emit more infrared radiation than the optical light they reflect, and astronomers in the past have used infrared surveys like the Wide-field Infrared Explorer (WISE) to search, but without success.
CfA astronomer Benjamin Schmitt was a member of a large team that used the 6-meter Atacama Cosmology Telescope (ACT) in Chile to search for Planet 9 at millimeter wavelengths. Although ACT was designed to study the cosmic microwave background radiation, its relatively high angular resolution and sensitivity makes it suitable for this type of search.
The astronomers scanned about 87% of the sky accessible from the Southern Hemisphere over a six year period, and then processed the millimeter images with a variety of techniques, including binning and stacking methods that might uncover faint sources but at the expense of losing positional information. Their search found many tentative candidate sources (about 3,500 of them) but none could be confirmed, and there were no statistically significant detections.
The scientists, however, were able to exclude with 95% confidence a Planet 9 with the above-estimated properties within the surveyed area, results that are generally consistent with other null searches for Planet 9. The results cover only about 10 to 20% of the possibilities, but other sensitive millimeter facilities are coming online and should be able to complete this search for Planet 9 as hypothesized.
More information:
Sigurd Naess et al, The Atacama Cosmology Telescope: A Search for Planet 9, The Astrophysical Journal (2021). DOI: 10.3847/1538-4357/ac2307
Provided by
Harvard University
Citation:
Still searching for Planet 9 (2022, March 14)
