This article examines the potential capability of “Starship” to be a space tug for the elliptic orbit departure and arrival processes. It is merely a first ballpark look, I would need more precise data for the orbital mechanics, and for the vehicle weight statement and engine performances, to obtain more reliable detail. But these results are “good enough” to show considerable promise!
The notion of space tug assist to reduce the delta-vee (dV)
requirements on interplanetary craft for hyperbolic departure from, and arrival to, Earth have been discussed in more detail in references
1 and 2. Some educated guesses for the
“Starship” weight statement and engine performances are given in references
3 and 4.
Presumed Input Data Values
For purposes of this preliminary look, it is the tug, not the unspecified interplanetary
craft, that is the focus. The following data were assumed about the
trajectories: a very extended elliptic
departure and arrival orbit, with
perigee altitude same as low circular orbit at about 300 km, a periapsis speed of about 10.9 km/s, which is very near Earth escape at that
altitude, and roughly a 9-day
period. Circular orbit is presumed to be
7.8 km/s at 300 km, with a 90 minute
period. That makes the dV requirement
from one orbit to the other just about 3.1 km/s, and I simply “budgeted” 0.2 km/s dV for any
rendezvous and docking requirements.
This is what I assumed about “Starship” for the purposes of
this study: inert (dry) mass 120 metric
tons, maximum-capacity propellant load
1200 metric tons, and the flaps and heat
shield left in place, pretty much as
with the prototypes that are test-flying now.
It flies with 6 Raptor-2 engines,
3 the sea level form, and 3 the vacuum
form. For the sea level engines in
vacuum, I presumed 230 metric tons-force
thrust and 355 sec Isp. For the vacuum
engines, I presumed 250 metric
tons-force thrust and 379 sec Isp. I
presumed a max turndown ratio of 4 for both variants.
Departure and Arrival Missions
The departure mission differs from the arrival mission, both in dV requirements and in the events
sequence. It is presumed that both vehicle
assembly and refueling take place at an unspecified facility located in low
Earth orbit (LEO), to which the tug
returns after assisting departures, and
with the interplanetary craft after assisting arrivals. Reaching such a facility from the Earth’s
surface is easiest, if it is located in
LEO at low inclination launching eastward.
At departure, the tug
is already coupled to the interplanetary craft,
so there is only the dV onto the ellipse, followed immediately by undocking and the
interplanetary craft firing its engines to reach hyperbolic speed. The unladen tug must then coast once about
the extended ellipse, and then finally supply
the dV’s for return to circular at the proper time-of-perigee, and for rendezvous
and docking with the unspecified facility there.
For arrivals, the
unladen tug must supply the dV’s for entry onto the ellipse at the proper ellipse
perigee time, plus a rendezvous and
docking budget for coupling to the interplanetary craft, which had already supplied the dV to enter
that ellipse from its hyperbolic approach.
The docked pair coast about the ellipse.
Then the laden tug must supply the dV’s for getting from the ellipse back
to circular, plus a rendezvous and
docking budget for returning to the unspecified facility.
Methods of Computation
I did this with a spreadsheet, embodying both rocket equation calculations
and a look at vehicle thrust/weight ratio for in-space accelerations. I simply presumed vehicle accelerations
outside the range of 0.2 to 4 gees as “unacceptable”. These are nothing but by-hand
pencil-and-paper-type calculations, just
automated for easy iteration with the spreadsheet.
The “first cut” single rocket equation calculation provided
performance data and a plot showing gross dV capability and accelerations for
variable “payload masses” representing the unspecified interplanetary
craft, and various selections of which
engines are operating. Those results are
given in Figure 1 below.
This is very unrealistic as a tug estimate, because the tug’s weight statements are
vastly different laden versus unladen,
but it does help to determine how many engines to use for acceptable accelerations, for various “payload” masses, including none.
When the weight statement does not change between burns, one may sum dV’s to a single overall dV
requirement (or not, as desired). When the weight statement does change, there must be a separate rocket equation
calculation for each weight statement,
and these calculations are linked by those weight statements, with the linkages consistent with the order
in which burns are made. I chose to
represent every tug burn, 3 for the
departure mission, and 4 for the arrival
mission.
The missions portion of the spreadsheet was set up for
arbitrary payload mass inputs, different
for each mission, with the option to
reduce propellant mass if excess dV resulted.
I used this to find the max payload masses for each mission, flown at full propellant load. Reduce the “payload” mass, and you may reduce the propellant load. However,
I did not explore that issue,
having no information at all about the unspecified interplanetary craft
that is the “payload” here.
Bear in mind that this is the first time I set up a tug
mission spreadsheet. It may get revised
as it gets used. But it is general
enough to investigate other possible tug designs, just using different inputs for vehicle
characteristics. An image of this
initial spreadsheet is given as Figure 2 below.
Discussion of Differing Mission Results
First, I used
the vehicle characteristics more-or-less representing the “Starship” prototypes
being test flown as of this writing.
Those masses include the heat shield and the aerodynamic control
flaps. This allows the vehicle to return
for repair and refurbishment, after
“something” wears out from repeated use,
presumably engines.
Second, the
mass of the unspecified interplanetary craft is much larger at departure than
at arrival. This is not as adverse a
result as it might seem. Any
interplanetary craft departing Earth will have a full load of propellants and
any other items for its mission, and
this will inherently be heavier. On
arrival back at Earth, it will be
essentially depleted of propellants and presumably unloaded of some
mission-related things, and so will
inherently be much lighter. That more-or-less
matches tug capability.
Third, for
departure tug missions, the docked pair
departs at fully-loaded mass, and the
larger mass ratio associated with the dV = 3.1 km/s burn onto the ellipse then reduces
that larger mass considerably. There is
no rendezvous and docking to worry about in this phase of the mission. The tug undocks from the interplanetary
craft, and then coasts around the
extended ellipse once, firing unladen
for a dV = 3.3 km/s to cover both getting back to circular and
rendezvous and docking with the unspecified orbital facility. That mass ratio applies to a much smaller
unladen mass, which is why the
propellant quantities are so small. And
THAT “laden-then-unladen” burn sequence is also the “magic” of booster flyback
recoveries for the Falcon and Starship systems! It does NOT work that
advantageously, for the “unladen-then-laden”
burn sequence.
Fourth, for
arrival tug missions, the tug departs
unladen from the unspecified orbital facility,
and must burn for a dV = 3.3 km/s to cover getting onto the ellipse and
rendezvous and docking with the unspecified interplanetary craft. That mass ratio applies to a smaller but
still-large mass at ignition, using a
lot of propellant. Then it gains
considerable “payload” mass after docking,
and must still supply dV = 3.3 km/s to cover getting back to
circular, plus rendezvous and docking
with the unspecified orbital facility,
while laden. That is another
large mass ratio reducing the burnout mass,
which is now required to be much larger,
being laden. And THAT unfavorable
reverse of the booster flyback “magic” is what limits the size of the arrival
payload mass!
Conclusions
First, “Starship”
as currently flown is a very large vehicle,
and so has a very large “payload” capacity if used as a departure
scenario tug assisting any unspecified departing interplanetary craft. These preliminary numbers as reported in the
first figure say the size of that “payload” is almost but not quite 500 metric
tons! The arrival “payload” capability
is much smaller at 175 metric tons, but
still quite considerable.
Second, crudely
speaking, this scales up or down with
the tug stage-only mass at its ignition:
that being the inert mass plus the propellant mass. We are presuming all the “payload” mass is
the unspecified interplanetary craft,
and none is inside the “Starship” cargo bay itself. Other stages or vehicles, fitted with the right controls and some sort
of on-orbit refueling plumbing, could
also serve this tug function, and still
be recovered for refueling and reuse. Such
might include the second stages of the Falcons,
the SLS upper stage, the Vulcan
second stage which is an upgraded Centaur,
and so on. There many
possibilities.
Third, that
being the case, it should not be very
difficult to develop multiple space tug designs out of these various upper
stages. The hardest part will be setting
up a space station facility in LEO that functions as both an assembly
facility, and a propellant refill
depot facility! And THAT is the most important result
here! We will need that LEO-based
facility to support any space tug-assist for any interplanetary craft. That is the real gateway to less-expensive
interplanetary travel, not some
hard-to-reach space station around the moon!
References 1 and 2 prove this conclusively.
Fourth, such
would also support lunar missions, as
well, since the extended ellipse could
apogee right near the moon’s orbit about the Earth. It is the 3-body effects when the moon is
there at craft apogee, that then turn
this into a figure-8 lunar transfer trajectory.
References
#1. G. W. Johnson, “Tug-Assisted
Arrivals and Departures”, posted to
“exrocketman” 12-1-2024.
#2. G. W. Johnson,
“Elliptic Capture”, posted to
“exrocketman” 10-1-2024.
#3. G. W. Johnson, “Rocket
Engine Calculations”, posted to
“exrocketman” 10-1-2022.
#4. G. W. Johnson,
“Reverse-Engineering Starship/Superheavy 2021”, posted to “exrocketman” 3-9-2021.
Use the archive tool on the left side of this “exrocketman”
page to quickly reach any of these references (or any other article posted
here). All you need is the date of
posting and the title. Click on the
year, then the month, and then the title if more than one article
was posted that month. This is far
easier than scrolling down.
Figures
Update 1-4-2025: added plot axis titles to the Figure 3 data plot made for Centaur-V as a tug. You may click on any figure to see them all enlarged. There is an X-out tab top right of that view, which takes you right back to this article.
Figure 1 – Spreadsheet Results For Both Gross-Overall
And Specific Mission Capabilities
Figure 2 – Image of the Initial Form of the Tug Spreadsheet
Set Up for “Starship”
Update (also) 1-2-2025:
I have started looking at other stages for possible tug
use, notably the Centaur, which uses higher-energy LOX-LH2
propellants. The Common Centaur stage
design uses a common bulkhead between the LOX and LH2 tanks, and single-wall thin stainless steel tank
walls that gain their strength from internal pressure by the “balloon effect”. The inter-tank bulkhead is two
stainless-steel membranes separated by some fiberglass hex as insulation, to keep the warmer LOX from heating the
colder LH2 too rapidly. Even so, the useful stage lifetime is only “hours
long”, limited by heating of the
hydrogen by the warmer oxygen, leading
to tank overpressure failure.
Centaur-III is the 3.05 m diameter form used on
Atlas-V, which only uses two RL-10
engines when lofting the Boeing CST-100 “Starliner”. The other applications are all one-engine, presumably underlying the data I found. The tank wall is 300-series stainless steel
0.020 inches (0.51 mm) thick.
Centaur-V has a larger hydrogen tank diameter, and comes in only the two-engine form, for use on the new Vulcan launcher. Centaur-V initially has only about 40% longer
stage lifetime, but it is said that it
will eventually have a few hundred percent longer lifetime, for much longer missions.
Centaur-III/Common Centaur simply does not have the
stage lifetime needed to serve as a tug on ellipses with multi-day periods! Eventually,
if the expected longer stage lifetimes turn out to be true, Centaur-V could serve as a tug! Tug duty could involve stage lifetimes in the
range of 10-days to 2 weeks, before
intervention is required to address hydrogen boiloff and overpressure risks.
I can only estimate, based on the “balloon pressure”
approximation, that total applied thrust
equals the “PA-kick load” associated with the tank pressure. Thus, the minimum operating tank pressure for the
1-engine Common Centaur stage would be P = Ftot/Atank = 22,300 lb/11,310 in2
= 2 psia min. For the 2-engine
form, that would be 4 psia min. The ideal tank failure hoop stress would the
ultimate tensile strength of 300-series stainless steel per Mil Handbook
5, which is about 95 ksi. The corresponding failure tank pressure is P
= 2 s t/D = 31-32 psi. However, it is rendered unusable by yielding, before reaching that value. This would actually be a bit lower for the
larger-diameter Centaur-V, nearer 20
psia.
Without an accurate empty mass for Centaur-V, I cannot run reliable tug performance
estimates for it! A “wild educated
guess” for the Centaur-V empty mass might be near 3200-3300 kg, based on a guess for the change in tank mass,
based on propellant masses, using “97% propellant”.
I ran these numbers as a rough cut for what a “long stage
life” Centaur-V might be able to do as a space tug for these elliptic arrival
and departure missions, using an
educated guess of 3.25 metric tons for the empty stage mass. The results are depicted in Figure 3, using the same spreadsheet as was used to
investigate “Starship” as a tug. I just
copied the “Starship” worksheet to another worksheet, and then changed all the input numbers, and finally re-iterated for max payload.
Unladen burns used only one of the two RL-10 engines on the
Centaur-V stage to limit vehicle gees. The results look good, except that the unladen burns for the
departure mission were around 6 gees. It
would probably be required to reduce from full thrust for that mission. That may reduce specific impulse a
little, which would in turn reduce max
payload a little.
Errors in the assumed stage empty mass subtract directly
from max payload capability on the tug missions.
Figure 3 – Results for Centaur-V As a Possible Tug (updated with axis titles 1-4-25)
Conclusion to this Update:
It would be fairly easy to install those changes needed to
use Centaur-V as a tug to assist interplanetary departures and arrivals, based from the unspecified facility in
LEO. The hardest part would be achieving
the necessary 2-week “stage life” to support extended ellipses to a 10 day
period. The biggest uncertainty
is the longer service life necessary for doing these missions routinely. The RL-10 engines were not intended to be “permanently”
re-startable.
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