Crab Nebula-how significant are we really?

At the core of the Crab Nebula, the close-up image reveals the remnants of a supernova, an exploding star. The inner region sends pulses of radiation  embedded in magnetic fields.
 
The neutron star at the very center of the Crab Nebula has about the same mass as our sun is compressed into a sphere that is only the size of a small town. Spinning 30 times a second, the neutron star shoots out detectable beams of energy that make it look like it’s pulsating.
 
The NASA Hubble Space Telescope snapshot is centered on neutron star which is a showcase for extreme physical processes and unimaginable cosmic violence. Bright wisps are moving outward from the neutron star at half the speed of light to form an expanding ring. 

The “heartbeat” radiation signature was first discovered in 1968, which became known as a class of supernova remnants called pulsars – or rapidly spinning neutron stars. Observations of the Crab supernova were recorded by Chinese astronomers in 1054 A.D. The nebula are bright enough to be visible in amateur telescopes.

The Crab Nebula is located a mere 6,500 light-years away in the constellation Taurus and spans only 10 light years across.  The USNO B1.0 catalog lists over one billion objects, and a bit less than half of them are galaxies. Only 88 have been given official names.

IN THAT CONTEXT: What is going on with us internally (our Way-of-Being) can’t be all that significant can it?