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Hulse–Taylor pulsar

Pulsar · Pulsar in the constellation Aquila

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About the Hulse–Taylor pulsar

The Hulse–Taylor pulsar is about 17,110 light-years from the Sun, so the light we see from it left about 17,110 years ago.

It is 20,684 light-years from the centre of the Milky Way.

The map lists it as a pulsar and shows it among the stars around the Sun, drawn on the plane of the Milky Way.

Its shrinking orbit gave the first evidence for gravitational waves (Nobel Prize 1993).

Key numbers

Distance17,110 light-years (5.25 kpc)
Distance from the Galactic centre20,684 light-years
Galactic coordinatesl = 49.97°, b = +2.12°
Spin period59 ms
Distance methodestimated from dispersion measure (uncertain by ~2×)

Data: ATNF Pulsar Catalogue v2.9.0.

Where it is

Its place in the universe, from the inside out: Sagittarius–Carina Arm › Milky Way › Local Group › Virgo Supercluster › Laniakea Supercluster › Observable universe.

Zoom out to see it in context: Local Arm, a view about 12,000 light-years across.

From Wikipedia

The Hulse–Taylor pulsar is a binary star system composed of a neutron star and a pulsar which orbit around their common center of mass. It is the first binary pulsar ever discovered.

Excerpt from the Wikipedia article Hulse–Taylor pulsar, licensed CC BY-SA 4.0.

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