Lunar eclipses happen at full moon, when the Sun, the Earth and the Moon are perfectly aligned : the Moon is then completely immersed in the terrestrial shadow created by the Sun.
On Monday, September 28th, this phenomenon will be particularly spectacular, since it will happen when the Moon is at perigee, i.e. at its closest distance from the Earth, roughly 357 000 km, instead of the average distance of 380 000 km. The apparent diameter of the Moon will thus be rather large : 33,48’. The last total eclipse of the Moon visible in France was in 2008.
The lunar orbit around the Earth is not a perfect circle, but an ellipse. Consequently, the Moon is not always at the same distance from the Earth.
Eclipse details
On that day, the Moon will be in the constelllation of Pisces, towards the south-west and will be relatively high in the metropolitan sky (about 28°). Visible right through the night, full Moon will occur at 04h 50m 30s.
All phases of the eclipse will be visible from France. At the Paris Observatory, the the Instittute for celestial mechanics and ephemeris calculations (l’Institut de mécanique céleste et de calcul des éphémérides - IMCCE) has computed the sequence, given below for French civil time :
- Entrance into the penumbra : 2h 11min 43s
- Entrance into the shadow : 3h 7min 9s
- Start of totality : 4h 11min 9s
- Full eclipse : 4h 47min 7s
- End of totality : 5h 23min 4s (Totality : 1h 11m 55s).
- Exit from the shadow : 6h 27min 4s
- Exit from the penumbra 7h 22min 31s
An indication of the overall state of the terrestrial atmosphere
The copper coloured aspect of the Moon is due to the fact that the red rays of the Sun are slightly dispered and deviated by the lower layers of the terrestrial atmosphere towards the centre of the shadow cone of the Earth.
The strength of the colour bears witness to the transparency of the terrestrial atmosphere ; if there is a great deal of dust, the Moon will be very dark, even invisible.
The more transparent the atmosphere, the more the colour of the eclipsed Moon will be coppery red or orange, with bluish edges. Conversely, the darker and greyer the Moon, with hardly any discernable details, the more the atmosphere is full of dust particles.
Thus, the general aspect of the Moon during the total eclipse furnishes a snapshot of the overall state of the terrestrial atmosphere !
A cycle of four consecutive eclipses
This total eclipse of the Moon is the fourth and last eclipse of a series of four consecutive total lunar eclipses which occurred in 2014 and 2015 ; the series of four total lunar eclipses is a relatively rare phenomenon, given that a succession of five total lunar eclipses does not exist. « It will have happened only 177 times during the 6000 years spanning the period 3 000 BC to 3000 AD It will happen again in 2032 and 2033 », added Pascal Descamps, Paris Obsservatory astronomer at the IMCCE.
Contact
- Pascal Descamps
Astronome de l’Observatoire de Paris (IMCCE)
01 40 51 22 68
Dernière modification le 21 décembre 2021