The comet’s dusty coma and tail is swept away from the Sun, which is towards the left of the image in this orientation. The tail can be seen to stretch at least 120 000 km in this relatively shallow image, and in deeper images, the coma alone is estimated to be at least 80–100 000 km across.

As each pixel in this image spans roughly 400 km at the comet, both Rosetta and the nucleus of 67P/C-G are too small to be resolved. But images like these provide important context information for the images taken by the spacecraft close to the comet, as its activity increases towards perihelion.

At the time the image was taken Rosetta and the comet were about 238 million km from the Sun; at perihelion on 13 August they will be between the orbits of Earth and Mars at a distance of about 186 million km from the Sun.

This image will be shown as part of the BBC Sky at Night TV programme in the UK on Sunday 14 June. The episode is a Rosetta special and includes interviews with a number of scientists discussing what we have learned about Comet 67P/C-G so far.