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— CH. 1 · DISCOVERY AND DETECTION —

S/2015 (136472) 1

~3 min read · Ch. 1 of 5
5 sections
  • Astronomers pointed the Hubble Space Telescope toward the Kuiper belt in April 2015. They used a specific instrument called the Wide Field Camera 3 to scan the darkness. The goal was not to find a moon but to study the dwarf planet Makemake itself. Images taken during that month revealed faint points of light near the main body. These points did not move with the background stars, indicating they were orbiting objects. The discovery team nicknamed this new object MK2 for internal use. On the 26th of April 2016, the Minor Planet Center officially announced the finding. This announcement confirmed that Makemake is not alone in its distant journey.

  • The satellite appears extremely faint when viewed through visible light telescopes. Its apparent magnitude measures 25 on the standard scale. This makes it 1,300 times dimmer than the parent dwarf planet Makemake. The difference in brightness between the two bodies reaches 7.80 magnitudes. Before this moon was found, data from the Spitzer and Herschel space telescopes showed strange thermal emissions. Makemake emitted more heat than expected for its size and visible brightness. Astronomers suspected extra dark surface area must be responsible for this excess radiation. That dark area could be distributed uniformly or hidden on satellites. The existence of S/2015 (136472) 1 supports the theory that dark satellites contribute to the heat signature. If the satellite has a uniform dark surface, its geometric albedo ranges from 2% to 4%. This reflectivity level matches the darkness of charcoal.

  • S/2015 (136472) 1 follows a likely circular path around its primary body. It completes one full orbit every 18 days. The distance from the center of the system is not precisely known but creates a specific semi-major axis. From Earth-based observatories, the orbital plane appears edge-on. This orientation means the satellite passes directly in front of or behind Makemake during certain times. Such alignment causes the moon to disappear into the glare of the larger dwarf planet most of the time. This geometry explains why earlier telescope observations failed to detect it. Scientists remain unsure if the object travels in a prograde or retrograde direction. The inclination suggests eclipses may have occurred years before January 2018. These events would happen when the moon crosses the line of sight from our planet.

  • The extreme darkness of the satellite offers clues about its history. Its gravity appears too weak to hold onto bright volatile ices. As these ices sublimate off the surface, they escape into space rather than staying attached. This process leaves behind a dark exterior layer similar to charcoal. The loss of bright material over time creates the low albedo observed today. If S/2015 (136472) 1 shares the same density as Makemake, it contributes less than 0.2% of the total system mass. This small fraction highlights how little matter this moon actually contains compared to its parent. The sublimation theory provides a physical explanation for the stark contrast between the two bodies. It suggests that size and gravity play critical roles in determining surface composition.

  • No official name exists for this distant companion yet. The designation S/2015 (136472) 1 serves as its provisional identifier. The prefix S indicates a satellite object. The year 2015 marks when the discovery occurred. The number 1 denotes it was the first satellite found that year. The code (136472) refers to the minor-planet number assigned to Makemake. Internally, the team called it MK2 to mean object 2 within the Makemake system. Future permanent names may come from figures in Easter Island mythology. This choice reflects the cultural origins associated with the dwarf planet itself. Until an official decision is made, astronomers will continue using the alphanumeric string. The Minor Planet Center maintains records of these designations for future reference.

Common questions

When was the moon of Makemake officially announced?

The Minor Planet Center officially announced the finding on the 26th of April 2016. This announcement confirmed that Makemake is not alone in its distant journey.

How does S/2015 (136472) 1 compare to Makemake in brightness?

S/2015 (136472) 1 measures 1,300 times dimmer than the parent dwarf planet Makemake. The difference in brightness between the two bodies reaches 7.80 magnitudes.

What is the orbital period of S/2015 (136472) 1 around Makemake?

S/2015 (136472) 1 completes one full orbit every 18 days. It follows a likely circular path around its primary body.

Why did earlier telescope observations fail to detect S/2015 (136472) 1?

Earlier telescope observations failed because the orbital plane appears edge-on from Earth-based observatories. This orientation means the satellite passes directly in front of or behind Makemake during certain times and disappears into the glare of the larger dwarf planet most of the time.

What explains the low albedo of S/2015 (136472) 1?

The extreme darkness results from gravity that is too weak to hold onto bright volatile ices. As these ices sublimate off the surface, they escape into space rather than staying attached, leaving behind a dark exterior layer similar to charcoal.