Astronomers have been concerned for years about how to explain why the Milky Way has fewer satellite galaxies than the standard dark matter model predicts. This is called the 'missing satellites problem'. To bring us closer to solving this problem, an international team of researchers used data from the Hyper Suprime-Cam (HSC) Subaru Strategic Program (SSP) to discover two completely new satellite galaxies.
These results have been published in the Publications of the Astronomical Society of Japan on June 8, 2024 by a team of researchers from Japan, Taiwan and America.
We live in a galaxy called the Milky Way, with other, smaller galaxies orbiting around it, called satellite galaxies. By studying these satellite galaxies, researchers can unravel mysteries surrounding dark matter and better understand how galaxies evolve over time.
“How many satellite galaxies does the Milky Way have? This has been an important question for astronomers for decades,” said Masahi Chiba, a professor at Tohoku University.
The research team recognized the possibility that there are likely many undiscovered, small satellite galaxies (dwarf galaxies) that are far away and difficult to detect. The powerful power of the Subaru telescope – which sits atop an isolated mountain above the clouds in Hawaii – is well suited to finding these galaxies. In fact, this research team previously found three new dwarf galaxies using the Subaru Telescope.
Now the team has discovered two more new dwarf galaxies (Virgo III and Sextans II). With this discovery, the total number of satellite galaxies found by different research teams is nine. This is still far fewer than the 220 satellite galaxies predicted by the standard theory of dark matter.
However, the footprint of the HSC-SSP does not cover the entire Milky Way. If the distribution of those nine satellite galaxies across the entire Milky Way is similar to what was found in the footprint captured by the HSC-SSP, the research team calculates that there may actually be closer to 500 satellite galaxies. Now we are faced with a “too many satellites problem”, rather than a “missing satellites problem”.
To better characterize the true abundance of satellite galaxies, more high-resolution images and analyses are needed. “The next step is to use a more powerful telescope that captures a wider view of the sky,” Chiba explains. “Next year, the Vera C. Rubin Observatory in Chile will be used to achieve that goal. I hope that many new satellite galaxies will be discovered.
