No joking: Get there in as little as 56 days, roundtrips as short as 153 days
https://phys.org/news/2026-04-interplanetary-shortcut- mars.html#google_vignette
and
https://gizmodo.com/astronomer-finds-a-shortcut-to-mars-by-following-an- asteroids-journey-through-space-2000752127
Some quotes:
" In a new study, Marcelo de Oliveira Souza of the State University of Northern Rio de Janeiro followed the predicted route of asteroid 2001
CA21 to look for a new path to reach Mars. The results, published in the journal Acta Astronautica, identify a course that would take
approximately 153 days for a round trip to the Red Planet and back. "
"The paper does not suggest that future missions must follow this
specific asteroid. Instead, it demonstrates a possible way to identify faster flight paths that traditional methods might miss. "This study illustrates how the well-defined plane geometry of a preliminary small-
body orbit can be employed as a methodological screening tool for rapid interplanetary transfer identification." "
Cryptoengineer <petertrei@gmail.com> wrote or quoted:
I took a quick look at both articles, and still have no idea as to how
the faster trip is obtained, and what observing asteroids have to do
with it.
The article links probably are clickbait based on
"Round-Trip Mars Missions in the 2031 Window: Feasible and
Extreme Scenarios Derived from CA21-Anchored Trajectories"
(2025-10-24) by Marcelo de Oliveira Souza.
On 5/3/2026 9:11 AM, Tony Nance wrote:
No joking: Get there in as little as 56 days, roundtrips as short as
153 days
https://phys.org/news/2026-04-interplanetary-shortcut-
mars.html#google_vignette
and
https://gizmodo.com/astronomer-finds-a-shortcut-to-mars-by-following-
an- asteroids-journey-through-space-2000752127
Some quotes:
" In a new study, Marcelo de Oliveira Souza of the State University of
Northern Rio de Janeiro followed the predicted route of asteroid 2001
CA21 to look for a new path to reach Mars. The results, published in
the journal Acta Astronautica, identify a course that would take
approximately 153 days for a round trip to the Red Planet and back. "
"The paper does not suggest that future missions must follow this
specific asteroid. Instead, it demonstrates a possible way to identify
faster flight paths that traditional methods might miss. "This study
illustrates how the well-defined plane geometry of a preliminary
small- body orbit can be employed as a methodological screening tool
for rapid interplanetary transfer identification." "
I took a quick look at both articles, and still have no idea as to how
the faster trip is obtained, and what observing asteroids have to do
with it.
Up till now, we've used Hohmann transfer orbits, which are optimized to reduce fuel consumption, which is considered the limiting factor.
We've long known that a faster trip can be done at the expense of more
fuel, and I don't see anything in these articles about the difference
in fuel consumption. So what is new?
I'm puzzled.
pt
"Round-Trip Mars Missions in the 2031 Window: Feasible and
Extreme Scenarios Derived from CA21-Anchored Trajectories"
(2025-10-24) by Marcelo de Oliveira Souza.
So what I take from this: What might be new is the restriction
of travel to a plane. The paper says,
ram@zedat.fu-berlin.de (Stefan Ram) wrote or quoted:
The article links probably are clickbait based on
"Round-Trip Mars Missions in the 2031 Window: Feasible and
Extreme Scenarios Derived from CA21-Anchored Trajectories"
(2025-10-24) by Marcelo de Oliveira Souza.
So what I take from this: What might be new is the restriction
of travel to a plane. The paper says,
. . .
|This work establishes, for the first time, a complete and
|dynamically coherent framework for round-trip Earth?Mars?Earth
|missions within the 2031 opposition, derived from the
|CA21-anchored astrodynamics approach. Using precise
|Lambert-based modeling and JPL Horizons ephemerides, two
|closed trajectories were identified and validated: an extreme
|33+30+90-day configuration and a feasible 56+35+135-day
|configuration. Together, they demonstrate that sub-year
|round-trip missions between Earth and Mars are not only
|geometrically possible but also dynamically consistent when
|constrained to the orbital plane of asteroid 2001 CA21.
|
|The extreme configuration defines the upper physical limit of
|heliocentric transfer performance, requiring energy levels
|beyond current propulsion capability but remaining fully
|compatible with classical gravitational mechanics.
|It illustrates what could be achieved by future high-specific-
|impulse systems or staged orbit-to-orbit architectures.
. . .
What that paper says.
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