Pulsar quadrant

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Pulsar quadrant
5bo2b$3b3o2b$2bo3b2o$o2bo2bob$o3bobob$o4bo2b2$2b3o! #C [[ THUMBSIZE 2 THEME 6 GRID GRIDMAJOR 0 SUPPRESS THUMBLAUNCH ]] #C [[ AUTOSTART ]] #C [[ THUMBSIZE 2 GPS 2 ]]
Pattern type Oscillator
Number of cells 18
Bounding box 9 × 9
Period 3 (mod: 3)
Heat 8
Volatility 0.46 | 0.46
Kinetic symmetry Unspecified
Discovered by David Buckingham
Year of discovery 1973

Pulsar quadrant (or pulse) is a period-3 oscillator that was found by David Buckingham in July 1973.[1] It consists of a quarter of the outer part of a pulsar stabilized by a cis-fuse with two tails.

Information on this oscillator's commonness with respect to other naturally-occurring patterns is currently unknown.

All strict still lifes with a population of 23 or fewer cells, all oscillators with 16 or fewer cells, and all spaceships with 35 or fewer cells are known to be glider-constructible. A glider synthesis of this object can be found in the infobox to the right.

See also

References

  1. ↑ Dean Hickerson's oscillator stamp collection. Retrieved on March 14, 2020.