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Supernova remnant

Tycho's Supernova Remnant

Also SN 1572 · 3C 10

Open in OuranosCompare its size
Tycho's Supernova Remnant — Chandra, X-ray
Chandra, X-ray. Credit: X-ray: NASA/CXC/Rutgers/K.Eriksen et al.. Licence: Public domain (NASA). Source

The remains of a white dwarf star that blew itself apart, seen from Earth as a new star in 1572.

Measured

Distance
about 8,900 light-years (published estimates 8,000–9,800)
Size
about 20 light-years across (approximate)
Constellation
Cassiopeia
Position (J2000)
RA 0h 25m 18s, Dec +64.15°

How far, from the Sun

About 8,900 light-years. To cross it:

  • Light8,900 years
  • Voyager 1's speed158 million years
  • Driving at 100 km/h96.1 billion years

Voyager 1 at the speed it moved outward over the year to 2026-10-25 (JPL Horizons). Driving: nonstop, never refuelling.

Facts

  • Tycho Brahe observed the supernova from November 1572; at its peak it rivalled Venus.
  • Light echoes from the blast confirmed in 2008 that it was a Type Ia supernova.
  • It helped overturn the old idea that the starry heavens never change.

Where this comes from

  • Tian & Leahy 2011, ApJ 729, L15 (kinematic distance 2.5–3.0 kpc)

Every catalogue Ouranos draws is credited on the credits page.