Hello space fans and welcome to another edition
of Space Fan News.
In this episode, remember that ultra diffuse
galaxy I told you about in SFNs 226 and 232?
You know, the one with NO dark matter?
Well turns out there is dark matter there
after all.
This was always a controversial finding, back
in SFN 226 I reported that the group who found
Dragonfly 44, an ultra diffuse galaxy with
very little dark matter in it, had also taken
a closer look at another galaxy, NGC1052-DF2
and wrote a paper, in Nature of all places,
announcing that according to their observations,
this galaxy rotated just like a galaxy would
if it had no dark matter at all in it.
Basically they were comparing the galaxies
luminous mass (the dust in radio, the hot
and cool gases in the infrared, and the stars
in infrared through visible) with the dynamical
mass which is inferred by looking at the motions
of easy to see things like globular clusters
within the galaxy to get a handle on things
we can’t see like black holes and dark matter.
If those two masses are close or the same,
there isn’t much dark matter there, and
according to the Dragonfly team, they were
close, so close that there couldn’t be any
dark matter there.
In most galaxies, those two masses are way
off, the luminous mass is much less than the
dynamical mass because dark matter is affecting
the motions of the star clusters.
So when this announcement came out it got
immediate blowback and in SFN 232 I outlined
the problems astronomers had with it.
To remind you, they claimed that the galaxy
was too dim and there is no way to measure
for sure how stable the orbits of the globular
cluster are, nor can we even tell if they
are gravitationally bound to the galaxy itself.
If the globular clusters aren’t really part
of the galaxy, then they can’t have anything
to contribute with respect to the dynamical
mass.
They also had a problem with the number of
globular clusters they claimed to have measured
in a galaxy this small.
The original authors claimed 1000 times more
than should be there in a galaxy this size.
Anyway watch SFN’s 226 and 232 for a more
complete accounting of the drama, there’s
links in the description and up here.
OK so now fast-forward to today.
Astronomers did a new analysis on this galaxy
and they found that, hang on a minute, this
thing is a lot closer to us that anyone thought.
The previous estimates and measurement of
dark matter in NGC1052-DF2 were reliant on
the distance to the galaxy - which they thought
was 64 million light years away.
So by looking at the galaxies using five different
methods some of which included photometry
with Hubble and the ground-based Gemini Telescopes
they recalculated the distance to NGC1052-DF2.
Now astronomers estimate that this ultra diffuse
galaxy is 42 million light years away and
I know what you’re thinking, “Why don’t
astronomers get their heads out of their collective
you-know-whats and just put 42 everywhere
they need a number?”
We’ve known for a long time now that 42
is all we need to know, we can stop doing
science now, we know the answer.
Anyway, this means that because the galaxy
is closer than we thought, the mass measurements
taken before - you know, the luminous and
dynamical masses - are smaller if the galaxy
is this far away.
Specifically, the amount of luminous mass
from the stars is reduced by about one quarter.
Stay with me here, if the amount of luminous
mass
is lower the proportion of normal matter is
smaller and the ratio of luminous to dynamical
is smaller, which means this galaxy is in
fact acting like all the others because the
difference between the two types of mass in
this galaxy is larger - and we have a galaxy
with dark matter in it.
For some reason, I can’t get the image of
an astronomer sticking their tongue out at
the first team out of my head here.
But let’s keep going, the lack of dark matter
was previously inferred by the slow movement
of star clusters but with the galaxy being
closer, it turns out they are moving at a
pretty normal rate, again just as if they
were in a galaxy that has dark matter in it.
[tongue]
Astronomers of this report say that with this
revised distance, the galaxy appears to be
a rather ordinary low surface brightness galaxy
with plenty of room for dark matter.
So I guess this means it’s not ultra diffuse,
I’m not sure about that part though.
Finally, according to the article I read on
this from Science Alert, there is another
galaxy NGC1052-DF4 which also appears to have
no dark matter and also appears to be 63 million
light years away, they are looking at that
galaxy too to see if it is closer than we
think.
Results so far suggest that it is, so dark
matter wins to live another day.
Well that’s it for this episode space fans,
thank you Deep Astronomy Patreon Patrons for
all of your support for what we do here, and
to OPT telescopes, if you need a scope, they
are a great company with good customer service
that I stand behind 100%
Thanks to all of you for watching and as always,
Keep Looking Up!
