Copyright 2023 Robert Clark
I was interested to read of a supposed asteroid passing near Earth turning out to be a Centaur upper stage launched in 1966. Because of the oddities of 'Oumuamua I wondered if the same could be true of 'Oumuamua as well.
This occurred to me in reading Avi Loeb discussing 'Oumuamua in his book, Extraterrestrial. He noted it had some small changing acceleration as if by outgassing. This would be the case if say a rocket stage developed a small hole and was outgassing the residual propellant left in the rocket after burnout even years later.
Because the Centaur rocket stage is bright white I wondered if such a stage could be visible in asteroid surveys at such a distance as 'Oumuamua was seen, about 25 million km at closest approach to Earth. The Centaur is only 3 meters wide by 12 meters long. 'Oumuamua's cylindrical shape is also notable. Also notable is Spitzer space telescope could not detect it in the infrared. The explanation given was a bright, i.e., reflective, object would heat up less, as it reflects much of the incident light, and so it was concluded Oumuamua was among the brightest of comets, assumed a comet because of the outgassing:
NASA Learns More About Interstellar Visitor 'Oumuamua
Small but Reflective
The new study also suggests that 'Oumuamua may be up to 10 times more reflective than the comets that reside in our solar system — a surprising result, according to the paper's authors. Because infrared light is largely heat radiation produced by "warm" objects, it can be used to determine the temperature of a comet or asteroid; in turn, this can be used to determine the reflectivity of the object's surface — what scientists call albedo. Just as a dark T-shirt in sunlight heats up more quickly than a light one, an object with low reflectivity retains more heat than an object with high reflectivity. So a lower temperature means a higher albedo.
https://solarsystem.nasa.gov/news/759/nasa-learns-more-about-interstellar-visitor-oumuamua/
But this would also be the case for a rocket stage painted white. Could the Centaur stage be visible at 25 million km distance by optical telescopes in being bright white?
But there is also the issue of the fact 'Oumuamua was on a trajectory suggesting escape velocity. In Loebs book he discusses that asteroids can be ejected from their parent systems by interactions with other planets in their systems. Then what occurred to me is whether a spent rocket stage could reach solar system escape velocity by the slingshot effect used on some of our spacecraft to get additional speed.
The possibility I was thinking about was the New Horizons mission. The spacecraft was given high initial speed by the stages sending it to the outer solar system but then additionally to that it was first directed towards Jupiter for a Jupiter slingshot effect.
The NH spacecraft was given escape velocity at Jupiter after the gravity assist though actually aimed at Pluto.
But suppose the Centaur, which was the upper stage to the Atlas V launcher, was also aimed at Jupiter in order to get NH there. There was an additional solid 3rd stage carrying the NH that got a slingshot effect from Jupiter. But it may have been the Centaur was aimed at Jupiter as well.
Now suppose the Centaur on reaching Jupiter happened to be so aimed, unintentionally perhaps, that Jupiter's orbital motion around the Sun plus the slingshot effect would be sufficient to give the Centaur solar system escape velocity.
But the aiming, whether unintentional or not, would have to be that rather than heading directly out of the solar system it would be headed towards the inner solar system.
But that’s where idea encounters problems. On calculating ‘Oumuamua’s trajectory backwards from its sighting near Earth, it appears to have had an incoming trajectory nearly perpendicular to the plane of the Solar System, at 123 degrees, as described by Adam Hibberd.
It doesn’t seem possible that the Centaur after it’s gravity assist at Jupiter would come into the inner solar system at such a high angle.
Another problem is the closeness of the flyby’s of Mercury, Venus, and Earth by ‘Oumuamua.
See discussion here:
Further strangeness of 'Oumuamua.
http://exoscientist.blogspot.com/2023/09/further-strangeness-of-oumuamua.html
It doesn’t seem reasonable that a rocket stage after doing a close flyby of Jupiter would subsequently also do ones of Mercury, Venus, and Earth.
So here’s another possibility. The Messenger spacecraft did multiple flybys of Mercury, Venus, and Earth on its trip to Mercury.
Then the upper stage that delivered Messenger on its trajectory to escape Earth may also have followed Messenger in its encounters with the inner solar system planets. The rocket that launched Messenger was the Delta II.
The Color of ‘Oumuamua.
Col-OSSOS: Colors of the Interstellar Planetesimal 1I/'Oumuamua
Michele T. Bannister, et al.
The Astrophysical Journal Letters, Volume 851, Number 2
Focus on the First Interstellar Small Body `Oumuamua
The grJ colors of 1I/'Oumuamua are at the neutral end of the solar system populations (Figure 3). About 15% of the TNOs have colors consistent with 1I/'Oumuamua, all in dynamically excited populations. 1I/'Oumuamua's color is also consistent with that of the less-red Jupiter Trojans, which are P type (Emery et al. 2011), and with Bus & Binzel (2002a) and DeMeo et al. (2009) X type in the asteroids, which encompasses the Tholen (1984) E, M, and P classifications. As its albedo is unknown, we do not describe 1I/'Oumuamua as consistent with the Tholen (1984) P type.
Notably, 1I/'Oumuamua does not share the distinctly redder colors of the cold classical TNOs (Tegler et al. 2003; Pike et al. 2017), which may be on primordial orbits. Nor is its color among the red or "ultra-red" colors of the larger TNOs on orbits that cross or are well exterior to the heliopause (Sheppard 2010; Trujillo & Sheppard 2014; Bannister et al. 2017). The cause of ultra-red coloration of these TNOs is unknown, but has been attributed to long-term cosmic-ray alteration of organic-rich surfaces (Jewitt 2002), such as would be expected during the long duration of interstellar travel.
https://iopscience.iop.org/article/10.3847/2041-8213/aaa07c/meta
An extreme form of the maneuver would be to approach a planet head-on at a speed v while the planet is moving directly toward us at a speed U (both speeds defined relative to the "fixed" Solar frame). If we aim just right we can loop around behind the planet in an extremely eccentric hyperbolic orbit, making a virtual 180-degree turn, as illustrated below. |
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The net effect is almost as if we "bounced" off the front of the planet. From the planet's perspective we approached at the speed U+v, and therefore we will also recede at the speed U+v relative to the planet, but the planet is still moving at (virtually) the speed U, so we will be moving at speed 2U+v. This is just like a very small billiard ball bouncing off a very large one. |