Results of an experimental study of binary recombination of para-and ortho-H + 3 ions with electrons are presented. Near-infrared cavity-ring-down absorption spectroscopy was used to probe the lowest rotational states of H + 3 ions in the temperature range of 77-200 K in an H + 3 -dominated afterglow plasma. By changing the para/ortho abundance ratio, we were able to obtain the binary recombination rate coefficients for pure para-H + 3 and ortho-H + 3 . The results are in good agreement with previous theoretical predictions.