A hypothetical configuration of planets that lack a central star, yet nevertheless
orbit a common point. A Klemplerer Rosette was first described by W. B.
Klemplerer in 1962.1 The concept was brought to widespread attention
by the science-fiction writer Larry Niven
in his novel Ringworld (1970).
In this novel, the use of a Klemplerer Rossette (or "Kemplerer Rosette"
as Niven spells it) is described by a member of the alien species known
as Pierson's Puppeteer:
| A pentagonal rosette as described
in Larry Niven's novel Ringworld. Image source: Wikipedia
"I had explained," said Nessus, "that our civilisation was
dying in its own waste heat. Total conversion of energy had rid us of
all waste products of civilisation, save that one. We had no choice but
to move our world outward from its primary."
"Was that not dangerous?"
"Very. There was much madness that year. For that reason it is famous
in our history. But we had purchased a reactionless, inertialess drive
from the Outsiders. You may have guessed their price. We are still paying
in installments. We had moved two agricultural worlds; we had experimented
with other, useless worlds of our system using the Outsider drive. In
any case, we did it. We moved our world."
"In short, we found that a sun was a liability rather than an asset. We
moved our world to a tenth of a light year's distance, keeping the primary
only as an anchor. We needed the farming worlds and it would have been
dangerous to let our world wander randomly through space. Otherwise we
would not have needed a sun at all."
"We had brought suitable worlds from nearby systems, increasing our agricultural
worlds to four, and setting them in a Kemplerer Rosette."
- Klemplerer, W. B. "Some Properties of Rosette Configurations of Gravitating
Bodies in Homographic Equilibrium". Astronomical Journal, vol.
67, number 3, 162-167 (1962).