For space, this quantity is equal to the Hubble constant squared over c squared times omega-M plus the mass density of the cosmological constant over the critical density minus one.
For space, this quantity is equal to the Hubble constant squared over c squared times omega-M plus the mass density of the cosmological constant over the critical density minus one. One form of this quantity is roughly equal to the inverse of the Hubble distance squared. For a parameterized space curve r(t) this quantity is equal to the magnitude of r prime crossed with r double primed over the magnitude of r prime raised to the third. One over the absolute value of this quantity is equal to its namesake radius. For a sphere, this quantity is equal to one over radius squared. For 10 points, name this quantity that measures how much an object deviates from being flat or a straight line.
For space, this quantity is equal to the Hubble constant squared over c squared times omega-M plus the mass density of the cosmological constant over the critical density minus one.
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