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Webb Telescope Reveals Black Hole's Galactic Scar - News Directory 3

Webb Telescope Reveals Black Hole’s Galactic Scar

October 9, 2025 Jennifer Chen Health
News Context
At a glance
  • Here's a breakdown of the details from the provided text, focusing on the key findings and ⁢details:
  • * ⁢A massive "contrail" - a faint,⁣ linear tail of gas and⁢ dust⁣ - within the ⁤spiral galaxy NGC 3627.
  • * Researchers believe⁤ a massive, compact object (likely a black hole, but potentially the nucleus of a dwarf galaxy) created the contrail.
Original source: livescience.com

Here’s a breakdown of the details from the provided text, focusing on the key findings and ⁢details:

What⁢ was discovered?

* ⁢A massive “contrail” – a faint,⁣ linear tail of gas and⁢ dust⁣ – within the ⁤spiral galaxy NGC 3627. This contrail is exceptionally long, stretching 20,000 light-years (one-fifth ⁢the width of the Milky ⁢Way).

What caused ‍the contrail?

* Researchers believe⁤ a massive, compact object (likely a black hole, but potentially the nucleus of a dwarf galaxy) created the contrail.
* The ⁢object is estimated to have a mass of 10 million times that of ‍our Sun.
* It was traveling⁤ at an incredibly high speed: 186 miles per ‍second (300 kilometers ⁤per second),exceeding the speed of the Parker Solar Probe.
* As the object moved through the galactic disk, it squeezed out⁢ gas, ⁢leaving ⁣the contrail ‍as a trace of its passage.

When did ⁣this happen?

* The ⁣contrail is estimated to ‍have formed around⁤ 20 million years ago, which⁣ is recent in astronomical terms.

How did they figure this out?

* The discovery was based on observations and a theoretical model ⁤developed in 2021.
* The turbulence ⁤within the contrail supports ‍the idea that it was created⁣ by a fast-moving,massive object.
* The features⁤ of the contrail allowed researchers to estimate the object’s mass and speed.

Source:

* ⁣ The research is available on arXiv: https://arxiv.org/abs/2509.20832

* ⁣The research was published in Monthly Notices of the Royal Astronomical Society: http://dx.doi.org/10.1093/mnras/stab735

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