Cosmological ghost condensate density ρ as a function of the scale factor a relative to its density ρ₀ today, at a = 1, for various values of the combination Q₀/𝒵₀. This is for m = 1 Mpc⁻¹, K_B = 0.1, H₀ = 70 km s⁻¹ Mpc⁻¹, and Ω₀ = 0.25. The ghost condensate follows a dust-like evolution only at late times. Larger values of m allow for dust-like evolution even at a = 10⁻⁴ but are in conflict with having MOND-like behavior around galaxies.