M1/NGC19523 The Crab – Supernova Remnant – An expanding cloud of dust from the explosion of a Supernova that was observed by the Japanese, Chinese in 1054 A.D. One of the brightest & conspicuous examples of a SN remnant. Back in 1054, the exploding star was so bright that it was visible during the daytime for several months. The Crab is located in the Constellation of Taurus. The cloud of dust is still expanding at about 1500KM per second. At the centre of the Crab is the collapsed core of the star that went supernova in 1054. This is now a Pulsar which is in fact a rapidly rotating and extraordinarily dense Neutron star, only a few KM in diameter and yet 1.4x the mass of our Sun, that emits a pulse of high energy X-ray radiation every 0.033 seconds as the Neutron star rotates at 30 times per second. The Crab is about 6 Light Years across and at a distance of 6,500 Light Years from Earth.
Below is a Hubble Space Telescope image of the Crab SN Remnant for comparison:
IC 434 The Horsehead Nebula – Slightly better resolved image (than last week) of the Horsehead Nebula in the Constellation of Orion. A Dark Nebula of dust silhouetted against the feint glow of Emission Nebula IC 434 behind.
Comet C/2014/Q2/Lovejoy – A visitor from the Oort Cloud in the outer Solar System and travelling at a speed of 133,000 Km per hour. Comet Lovejoy is known as a long period comet and it orbits the Sun once every 11,000 years. It comes closest to the Sun on 30th January at a distance of 1.3 Astronomical Units or 1.3 x the distance between the Sun and the Earth. It is currently about 95 Million KM from Earth and now passing through the Constellation of Aries.
Lovejoy is the brightest comet for some time at visual magnitude of about 5.0, just about visible in binoculars from London. Difficult to see in image below but I think a feint tail is detectable to the upper left of the comet’s head.