Makemake and Its Moon
Makemake and Its Newly Discovered Moon (Artist's Concept)
Peering to the outskirts of our solar system, NASA's Hubble Space Telescope has spotted a small, dark moon orbiting Makemake, the second brightest icy dwarf planet — after Pluto — in the Kuiper Belt.
The moon — provisionally designated S/2015 (136472) 1 and nicknamed
MK 2 — is more than 1,300 times fainter than Makemake. MK 2 was seen
approximately 13,000 miles from the dwarf planet, and its diameter is
estimated to be 100 miles across. Makemake is 870 miles wide. The dwarf
planet, discovered in 2005, is named for a creation deity of the Rapa
Nui people of Easter Island.
The Kuiper Belt is a vast reservoir of leftover frozen material from
the construction of our solar system 4.5 billion years ago and home to
several dwarf planets. Some of these worlds have known satellites, but
this is the first discovery of a companion object to Makemake. Makemake
is one of five dwarf planets recognized by the International
Astronomical Union.
The observations were made in April 2015 with Hubble's Wide Field
Camera 3. Hubble's unique ability to see faint objects near bright
ones, together with its sharp resolution, allowed astronomers to pluck
out the moon from Makemake's glare. The discovery was announced today
in a Minor Planet Electronic Circular.
The observing team used the same Hubble technique to observe the moon
as they did for finding the small satellites of Pluto in 2005, 2011,
and 2012. Several previous searches around Makemake had turned up
empty. "Our preliminary estimates show that the moon's orbit seems to
be edge-on, and that means that often when you look at the system you
are going to miss the moon because it gets lost in the bright glare of
Makemake," said Alex Parker of the Southwest Research Institute,
Boulder, Colorado, who led the image analysis for the observations.
A moon's discovery can provide valuable information on the
dwarf-planet system. By measuring the moon's orbit, astronomers can
calculate a mass for the system and gain insight into its evolution.
Uncovering the moon also reinforces the idea that most dwarf planets have satellites.
"Makemake is in the class of rare Pluto-like objects, so finding a
companion is important," Parker said. "The discovery of this moon has
given us an opportunity to study Makemake in far greater detail than we
ever would have been able to without the companion."
Finding this moon only increases the parallels between Pluto and
Makemake. Both objects are already known to be covered in frozen
methane. As was done with Pluto, further study of the satellite will
easily reveal the density of Makemake, a key result that will indicate
if the bulk compositions of Pluto and Makemake are also similar. "This
new discovery opens a new chapter in comparative planetology in the
outer solar system," said team leader Marc Buie of the Southwest
Research Institute, Boulder, Colorado.
The researchers will need more Hubble observations to make accurate
measurements to determine if the moon's orbit is elliptical or
circular. Preliminary estimates indicate that if the moon is in a
circular orbit, it completes a circuit around Makemake in 12 days or
longer.
Determining the shape of the moon's orbit will help settle the
question of its origin. A tight circular orbit means that MK 2 is
probably the product of a collision between Makemake and another Kuiper
Belt Object. If the moon is in a wide, elongated orbit, it is more
likely to be a captured object from the Kuiper Belt. Either event would
have likely occurred several billion years ago, when the solar system
was young.
The discovery may have solved one mystery about Makemake. Previous
infrared studies of the dwarf planet revealed that while Makemake's
surface is almost entirely bright and very cold, some areas appear
warmer than other areas. Astronomers had suggested that this
discrepancy may be due to the sun warming discrete dark patches on
Makemake's surface. However, unless Makemake is in a special
orientation, these dark patches should make the dwarf planet's
brightness vary substantially as it rotates. But this amount of
variability has never been observed.
These previous infrared data did not have sufficient resolution to
separate Makemake from MK 2.
The team's reanalysis, based on the new
Hubble observations, suggests that much of the warmer surface detected
previously in infrared light may, in reality, simply have been the dark
surface of the companion MK 2.
There are several possibilities that could explain why the moon would
have charcoal-black surface, even though it is orbiting a dwarf planet
that is as bright as fresh snow. One idea is that, unlike larger
objects such as Makemake, MK 2 is small enough that it cannot
gravitationally hold onto a bright, icy crust, which sublimates,
changing from solid to gas, under sunlight. This would make the moon
similar to comets and other Kuiper Belt Objects, many of which are
covered with very dark material.
When Pluto's moon Charon was discovered in 1978, astronomers quickly calculated the mass of the system. Pluto's mass was hundreds of times smaller than the mass originally estimated when it was found in 1930. With Charon's discovery, astronomers suddenly knew something was fundamentally different about Pluto. "That's the kind of transformative measurement that having a satellite can enable," Parker said.
Contact
Donna Weaver / Ray Villard
Space Telescope Science Institute, Baltimore, Maryland
410-338-4493 / 410-338-4514
dweaver@stsci.edu / villard@stsci.edu
Alex Parker
Southwest Research Institute, Boulder, Colorado
360-599-5346
alex.parker@swri.org
Source: HubbleSite
