Makemake: The Distant Red World

Makemake: The Distant Red World

Explore the mysterious reddish dwarf planet in the outer reaches of our solar system

What is Makemake?

Makemake is a dwarf planet located in the Kuiper Belt, a region of icy bodies beyond the orbit of Neptune. It is the second-brightest object in the Kuiper Belt as seen from Earth, after Pluto.

With a diameter of approximately 1,430 km, Makemake is about two-thirds the size of Pluto. It takes about 305 Earth years to complete one orbit around the Sun.

Makemake is named after the creator god in the mythology of the Rapa Nui people of Easter Island. The name reflects its discovery around Easter time in 2005.

Artistic representation of Makemake's reddish surface

Artistic representation of Makemake showing its distinctive reddish color

Discovery and Naming

Palomar Observatory in California Where Makemake was discovered

Palomar Observatory where Makemake was discovered

Makemake was discovered on March 31, 2005, by a team led by Michael E. Brown at the Palomar Observatory in California. The discovery was announced to the public on July 29, 2005.

Initially designated as 2005 FY9, the object was later given the minor planet number 136472. In July 2008, it was officially named Makemake by the International Astronomical Union.

The name Makemake comes from the mythology of the Rapa Nui people of Easter Island, where Makemake is the creator of humanity and the god of fertility. The name was chosen partly because the discovery was made just after Easter.

March 31, 2005

Makemake discovered by Michael Brown's team at Palomar Observatory

July 29, 2005

Discovery announced to the public along with Eris and Haumea

2006

Initial studies reveal Makemake's reddish color and methane ice surface

July 2008

Officially named Makemake by the International Astronomical Union

April 2016

Discovery of Makemake's moon, MK2, announced by Hubble Space Telescope

The Mysterious Red Color

Makemake has a distinctly reddish color in visible light, similar to Pluto but slightly less red. This coloration is one of its most distinctive features.

The red color is believed to be caused by tholins - complex organic molecules that form when methane is exposed to solar ultraviolet radiation. These tholins give Makemake its characteristic reddish-brown appearance.

Spectroscopic studies have shown that Makemake's surface is covered with large grains of methane ice, along with possible traces of nitrogen and ethane ice. The methane on the surface appears to be in its pure form rather than dissolved in nitrogen as on Pluto.

Pluto (Reddish-Brown) Makemake (Deeper Red) Comparison of Surface Colors

Comparison between Makemake's red color and Pluto's reddish-brown surface

Why Makemake is Red

The reddish color of Makemake comes from complex organic compounds called tholins that form on its surface. These tholins are created when methane (CH₄) is exposed to ultraviolet radiation from the Sun.

The process begins when solar radiation breaks down methane molecules, which then recombine into more complex hydrocarbons. These hydrocarbons continue to polymerize, eventually forming the reddish tholin compounds that color Makemake's surface.

Unlike Pluto, where nitrogen dominates the surface ice, Makemake appears to have large areas of nearly pure methane ice. This difference in composition affects the specific color and appearance of the two dwarf planets.

The distribution of tholins on Makemake's surface is not uniform, suggesting variations in surface composition and possibly seasonal changes as Makemake moves along its elliptical orbit.

Physical Characteristics

Makemake orbits the Sun at an average distance of 45.8 AU, taking about 305 Earth years to complete one orbit. Its orbit is moderately eccentric and inclined relative to the plane of the solar system.

Makemake has one known moon, designated S/2015 (136472) 1 and nicknamed MK2. This small moon was discovered in 2016 by the Hubble Space Telescope and is estimated to be about 175 km in diameter.

Observations suggest that Makemake has a very low average density of about 1.7 g/cm³, indicating it is composed largely of ices with only a small rocky core.

Makemake's Orbit Sun Makemake MK2 Diagram showing Makemake's orbit and its moon MK2

Diagram showing Makemake's orbit and its moon MK2

Size and Mass

Diameter: Approximately 1,430 km

Mass: ~3 × 10²¹ kg

Density: ~1.7 g/cm³

Orbital Characteristics

Average distance from Sun: 45.8 AU

Orbital period: 305 Earth years

Rotation period: 7.77 hours

Physical Properties

Surface temperature: ≈ -243°C

Albedo: 0.77 - 0.90

Surface composition: Methane, nitrogen, ethane ices

Atmosphere and Surface

Makemake's Temporary Atmosphere Forms when closer to the Sun

Makemake may develop a temporary atmosphere when closer to the Sun

Makemake likely has a very thin, transient atmosphere that forms when the dwarf planet is closest to the Sun in its orbit. As it moves away from the Sun, this atmosphere likely freezes and collapses back onto the surface.

Observations during a stellar occultation in 2011 provided evidence for this temporary atmosphere. The data suggested that if Makemake has an atmosphere, it must be highly tenuous, with a surface pressure less than 1 billionth of Earth's atmospheric pressure.

The primary component of Makemake's potential atmosphere is likely methane gas, which sublimes from the surface ice when temperatures increase during the dwarf planet's closest approach to the Sun.

Surface Features and Composition

Makemake's surface appears to be relatively uniform compared to other dwarf planets like Pluto. However, recent observations have revealed some variations in color and brightness across its surface.

The surface is dominated by methane ice, with spectral evidence suggesting the presence of large methane grains. This is different from Pluto, where nitrogen is the dominant surface ice.

Ethane and tholins are also likely present on Makemake's surface. The tholins are responsible for the dwarf planet's reddish color, while the ethane may form through photochemical processes involving methane.

The discovery of Makemake's moon, MK2, has provided new insights into the dwarf planet's mass and density, helping scientists better understand its internal structure and composition.

Makemake

Diameter: 1,430 km

Surface: Methane ice with tholins

Atmosphere: Transient, methane-based

Pluto

Diameter: 2,377 km

Surface: Nitrogen ice with methane

Atmosphere: Nitrogen with methane

Eris

Diameter: 2,326 km

Surface: Methane ice

Atmosphere: Transient, methane-based