A Milky Way and Andromeda galaxy collision may not be happening after all

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A 100,000 light-year separation leads to a collision. Credit: NASA / ESA
A 100,000 light-year separation leads to a collision. Credit: NASA / ESA

The chance that our Milky Way Galaxy will collide with the Andromeda Galaxy may not be as certain as previously thought, according to Aussie researchers, who say that a new simulation has found a 50% chance that there will be no collision between the two galaxies in the next 10 billion years. The collision of our galaxy and Andromeda in about five billion years has been suggested as a high likelihood scenario, with the resulting new galaxy already dubbed 'Milkomeda', however the authors suggest that the gravitational pull of the Large Magellanic Cloud was not considered in previous analyses and a merger between the Milky Way and the Large Magellanic Cloud is is almost certain within the next two billion years, they say.

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From: Springer Nature

Astronomy: Milky Way may escape galactic collision with Andromeda *IMAGE*

The likelihood of a collision between the Milky Way and its neighbouring galaxy Andromeda may be smaller than previously thought, according to a new simulation described in Nature Astronomy.

The Milky Way is moving through the Universe and its path is influenced by the combined gravitational pulls of nearby galaxies, such as Andromeda, the Triangulum galaxy and the Large Magellanic Cloud. As such, previous research has suggested for over a decade that the Milky Way has a high likelihood of colliding with Andromeda, forming a new galaxy dubbed ‘Milkomeda’, in approximately five billion years.

Till Sawala and colleagues simulated the Milky Way’s movement through the Universe over the next 10 billion years using updated data from the Gaia and Hubble telescopes and revised estimates of the masses of local galaxies. They found that there is an approximately 50% chance that there will be no Milky Way–Andromeda collision in that time period. The authors suggest that including the gravitational pull of the Large Magellanic Cloud — a smaller galaxy orbiting the Milky Way — in the calculations, which was not considered in previous analyses, and accounting for uncertainties, could explain the reduced probability. Sawala and colleagues also suggest that a Milky Way–Large Magellanic Cloud merger is almost certain within the next 2 billion years, before any potential collision with Andromeda.

The authors note that even using the most up-to-date data, there is still some uncertainty about how the Milky Way–Andromeda system will evolve, and that future data from the Gaia telescope could help produce a more accurate simulation.

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Three future scenarios for Milky Way & Andromeda encounter
Three future scenarios for Milky Way & Andromeda encounter
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conference:
Nature Astronomy
Research:Paper
Organisation/s: International Centre for Radio Astronomy Research (ICRAR)
Funder: J.D. and J.H. are supported by the Research Council of Finland (Grant No. 354905). T.S., J.H. and P.H.J. are also supported by the Research Council of Finland (Grant No. 339127). J.D. is supported by an Erasmus+ grant. T.S. and C.S.F. are supported by the European Research Council through the Advanced Investigator Grant DMIDAS (Grant No. GA 786910) and an STFC Consolidated Grant (Grant No. ST/T000244/1). P.H.J., A.K., A.R. and R.W. also acknowledge support from the European Research Council (Consolidator Grant KETJU No. 818930). This work used facilities hosted by the CSC-IT Centre for Science, Finland, and the DiRAC@Durham facility, managed by the Institute for Computational Cosmology on behalf of the STFC DiRAC HPC Facility (www.dirac.ac.uk) and funded by BEIS capital funding (STFC Capital Grant Nos. ST/K00042X/1, ST/P002293/1, ST/R002371/1 and ST/S002502/1), Durham University and the STFC (Operations Grant No. ST/R000832/1). DiRAC is part of the UK national e-Infrastructure. We thank the authors of the open-source software listed in ʽCode Availabilityʼ.
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