CubSat Exploration
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Transcript CubSat Exploration
CubSat Exploration
A plan for finding new exoplanets in
the Beta Pictoris system
The Target: Beta Pictoris
Artist's conception of the planet-forming disk around the
star Beta Pictoris. The carbon-rich gas disk is fed by the
debris from small colliding bodies and the evaporation
of comets. Credit: NASA / FUSE / Lynette Cook
Beta Pictoris is a fourth
magnitude star, with a
distance of 63.4 light years
and an age of only 8–20
million years.
The star itself is 1.75 times
as massive and 8.7 times
as luminous as our Sun,
making it a fourth
magnitude star.
The star is surrounded by a
debris disk, which is edgeon to our observations from
Earth, making it easier to
study the contents of the
disk itself.
The Planet: β-Pic B
The European Southern Observatory
confirmed the presence of a planet
orbiting within Beta Pictoris' disk.
This was done through the use of direct
imaging — a usually difficult method to
use when it comes to exoplanets.
Beta Pic b has a mass between 4 and
11 Jupiter masses and a radius about
65 percent larger than Jupiter's. The
planet orbits at a distance of 9 AU from
the star Beta Pictoris, with a low
eccentricity and a period of roughly 20
years. In comparison, Bets Pic b’s orbit
is just under the size of Saturn’s around
our own sun.
The Plan: Transit Photometry
Since the debris disk around Beta
Pictoris is edge-on and not too
dense we can easily observe
objects that pass in front of the star
By measuring the light curve we
can potentially see dips in the star’s
brightness when a planet passes in
front of the star
Any dip in the curve must be at
least three times the noise (sigma)
in the stellar brightness
measurements
We will calculate for detection of at
least 3 sigma
The Parameters: Our Formulas
Transit Depths - The percentage of light
blocked by the planet passing in front of the
star is proportionate to their relative sizes
Scatter Noise - The noise must be no more
than a third of the transit depth to be
detected and acknowledged as a planet
Number of Photons - To reduce the noise of
the star we must collect a certain number of
photons
Time for Detection - The time needed to
collect the number of photons given the
stellar flux and efficiency of the telescope
Semi-Major Axis - Assuming that the
cubesat lasts a year we will be looking
within a distance of 0.597 AU
𝑅𝑝
2
𝜎≈(
)
𝑅∗
𝜆=𝜎 3
𝑁𝑝ℎ = 1
𝜆2
𝑁𝑝ℎ
∆𝑡 =
𝐹𝑥 ∗ 𝜂
2
𝐺𝑀𝑝
𝑎3 =
4𝜋 2
The Results: We Can Detect New
Planets
This graph gives us
our measure of 3
sigma for a planet
of a certain size
Results Cont.
This graph tells us
how many photons
will reduce the
stellar noise
enough to see the
dip
Results Cont.
This graph tells us
hoe long our
cubesat will have
to observe in order
to make accurate
detections
The Future: Next Steps
The next step will
be designing an
instrument that can
achieve the
requirements we
have set.
We will have to
either buy or
develop a
telescope and
detector with the
precision to detect
planets of at least
Neptune size up to
Super Jupiters.
The NAC Program
My experience with my peers and mentors
The Mentor: Dr Aki Roberge
I had the pleasure of working with
Dr. Aki Roberge, a NASA scientist
at the Goddard Space Flight
Center
Her fields of study are Exoplanets
and Stellar Astrophysics
She received her B.S. in Physics
at Massachusetts Institute of
Technology, her M.A. in Physics at
John Hopkins University and her
PhD in Astrophysics at John
Hopkins University
Her thesis was on Ultraviolet
Spectroscopy of Circumstellar
Disks
The Peers: My Dear Friends
One great aspect of the
NAC program is that we
have a group of other
students to converse,
grow and bond with.
Every week we would
meet up for project
updates and to discuss
which events we would
be attending.
Having a group of peers
helps with feeling more
accepted in the
internship. Makes it a
safe place.
The Fun: Our Trips and Experience
We also had the
pleasure of taking trips
around the area and
being involved in many
events over the summer.
We attended the Young
Astronomers meeting at
Catholic University, the
Indigenous Youth Day
Science Fair, and took a
tour of University of
Maryland College Park
and their new Astronomy
building.