NASA reveals Kerberos – the last of Pluto’s moons

This image of Kerberos was created by combining four individual Long Range Reconnaissance Imager (LORRI) pictures taken at a range of 396,100 kilometres from Kerberos. The moon appears to have a double-lobed shape, approximately 12 kilometres across in its long dimension and 4.5 kilometres in its shortest dimension.

NASA has completed the family portrait of Pluto and its moons with images of the tiny Kerberos sent back to Earth this week by spacecraft New Horizons – and it is nothing like what scientists were expecting. The satellite is small with a highly-reflective surface, rather than massive with a dark surface, as had been theorised. 

“Once again, the Pluto system has surprised us,” said New Horizons Project Scientist Hal Weaver, of the Johns Hopkins University Applied Physics Laboratory in Laurel, Maryland.

The new data show that Kerberos appears to have a double-lobed shape, with the larger lobe approximately eight kilometres across and the smaller lobe approximately 5 kilometres across.

Its unusual shape could be the result of a merger of two smaller objects.

Hubble Space Telescope images in the past have been used to “weigh” Kerberos by measuring its gravitational influence on its neighbouring moons. That influence was surprisingly strong, considering how faint Kerberos was. They theorised that Kerberos was relatively large and massive, appearing faint only because its surface was covered in dark material.

But the small, bright-surfaced Kerberos revealed here shows that the idea was incorrect, but scientists do not know why.

“Our predictions were nearly spot-on for the other small moons, but not for Kerberos,” said New Horizons co-investigator Mark Showalter, of the SETI Institute in Mountain View, California.

Completing the family portrait of Pluto’s moons. This composite image shows a sliver of Pluto’s large moon, Charon, and all four of Pluto’s small moons, as resolved by the Long Range Reconnaissance Imager (LORRI) on the New Horizons spacecraft. All four small moons have highly elongated shapes, a characteristic thought to be typical of small bodies in the Kuiper Belt.