Spinning hourglass object may be the first of many to be discovered in the Kuiper belt

Oct 03, 2011

(PhysOrg.com) -- The bizarre, hourglass-shaped Kuiper belt object 2001QG298 spins round like a propeller as it orbits the Sun, according to an astronomer from Queens University Belfast. The discovery that the spinning object is tilted at nearly 90 degrees to the ecliptic plane is surprising, and suggests that this type of object could be very common in the Kuiper belt. The finding will be presented by Dr Pedro Lacerda at the Joint Meeting of the European Planetary Science Congress and the Division for Planetary Sciences in Nantes, France, on 3 October 2011.

The (KBOs) the sun beyond and are the best preserved leftovers of the formation of the planets. 2001QG298 is a remarkable KBO made up from two components that orbit each other very closely, possibly touching.

"Imagine that you glue two eggs together tip to tip – that's approximately the shape of 2001QG298. It looks a bit like an hourglass," says Lacerda.

The strange shape of 2001QG298 was uncovered by Dr Scott Sheppard and Prof David Jewitt in 2004. They noticed that 2001QG298's apparent brightness periodically tripled every 7 hours or so.

This video is not supported by your browser at this time.
This video shows an artistic rendering of 2001QG298 as seen from earth between 2004 and 2020. It shows how the observing angle and the lightcurve change as the object moves in its orbit along the sun

"The object is so distant that we cannot resolve its shape. But this brightness oscillation, called a lightcurve, reveals the strange shape of 2001QG298 as it spins round. The object appears faint at times because one lobe is hidden behind the other, so less area is reflecting sunlight. As the hidden component rotates back into view, we can see the full hour-glass shape. The reflecting area increases and the whole thing looks brighter," explains Lacerda.

However, Lacerda’s new study shows that 2001QG298's rotation is almost perpendicular to the plane of its orbit around the sun. Lacerda re-measured the object's lightcurve in late 2010 and noticed that it had changed from Sheppard and Jewitt’s observations. The lightcurve variation has become visibly shallower.

“It was impossible to tell from the original observations if the rotation and the orbital plane of 2001QG298 were aligned or perpendicular i.e. whether the object spun round horizontally like the blades on a helicopter or rotated vertically like the of an aeroplane. The changes to the lightcurve variation show that it must be approximately vertical. As 2001QG298 moves round in its orbit of The sun, our viewing geometry of the ‘propeller’ is gradually opening out from edge-on to seeing the whirling ‘blades’ full-face. This means that more of the reflecting surface is becoming visible at all times so the variation in the object’s brightness gradually disappears,” says Lacerda.

The most important consequence of this finding is that it suggests that this type of double KBO could be very common. When in 2004 Sheppard and Jewitt found 2001QG298 in a sample of 34 KBOs they realised that they were fortunate to spot its binary nature – if it had not happened to be edge-on at the time of their observations, they would not have seen the extreme lightcurve variation. They estimated that approximately 10% of all KBOs are contact binaries, assuming that their tilts are random.

However, Lacerda believes that the tilts of contact binaries may not actually be random and that objects similar to 2001QG298 could be even more common.

"It was a surprise to find that 2001QG298 is inclined by 90 degrees, but that's not the first time we’ve seen this in a contact binary,” he speculates. “There is another famous doublet object, a large Trojan asteroid called 624 Hektor. That object is also tilted almost 90 degrees."

If contact binaries tend to be highly tilted then the chance of spotting their characteristic variable lightcurve is even smaller – only about twice per orbit. The identification of one in a small sample implies that contact binaries may be even more abundant than Sheppard and Jewitt first thought. Lacerda estimates that as many as 25% of KBOs are contact binaries.

"If contact binaries do tend to be very inclined that may be telling us something about how these objects formed," concludes Lacerda.

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User comments : 9

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HannesAlfven
1.4 / 5 (14) Oct 03, 2011
Within the plasma cosmology view, the bipolar morphology is the pinching of two or more filamentary plasmas. Within the laboratory, plasma filaments exhibit long-range attraction and short-range repulsion with one another.

The reason that you see the pinch and not the attached filaments is because the current density reaches a critical level at the pinch which transitions the plasma from dark to glow modes. The dark mode plasmas tend to be more visible at the 21-cm wavelength. At that wavelength, fuzzy algorithms can identify more of the characteristic pinwheel and tubular structures which we see with laboratory plasmas conducting electrical currents.

Until students are trained in the electrical plasma-based framework, objects like these will continue to perplex astronomers and theorists alike. There should be no heresy in claiming that electricity flows through space. Rather than ignoring the claim, we should investigate it, elaborate it and problem-solve from it.
tadchem
4.7 / 5 (6) Oct 03, 2011
There's something VERY familiar about a 'spinning hourglass.'
May I be the first to suggest the informal name "Microsoft?"
xeno
5 / 5 (1) Oct 03, 2011
i wish this was a derelict alien spaceship
macsglen
not rated yet Oct 03, 2011
There's something VERY familiar about a 'spinning hourglass.'
May I be the first to suggest the informal name "Microsoft?"

Probably wouldn't hurt their reputation; they're pretty efficient about that themselves.
Oh, and -- you might want to ask them first.
CaliforniaDave
5 / 5 (2) Oct 03, 2011
The video is very interesting but what the hell is the soundtrack supposed to represent? The noise it makes as it plows through the vacuum? Please let's have a bit of scientific accuracy here...
lbentil
not rated yet Oct 04, 2011
It's an interesting object, I wonder how this supposed shape was formed. Will there be better luck in better perceiving this object with the New Horizons spacecraft once it reaches the Kuiper Belt?
omatumr
1.1 / 5 (7) Oct 04, 2011
Spinning hourglass object may be the first . . .


Observation to confirm element-isotope-nuclear-seismology record: An exploding star produced the Solar System [1-7]

1. "Xenon in carbonaceous chondrites", Nature 240, 99-101 (1972)

2. "Excess 26Mg in the Allende meteorite," Nature 251, 495-497 (1974)

3. "Elemental and isotopic inhomogeneities in noble gases: The case for local synthesis of the chemical elements", Trans MO Acad Sci 9, 104-122 (1975)

4. "Strange xenon, extinct super-heavy elements, and the solar neutrino puzzle", Science 195, 208-209 (1977)

5. "Is the Sun a pulsar?" Nature 270, 159-160 (1977)

www.nature.com/na...9a0.html

6. The end of dogmas on the formation of the Solar System, Nature 303, 286-286 (1983)

http://tallbloke....1983.pdf

7. Solar abundances of the elements, Meteoritics 18, 209-222 (1983)

www.omatumr.com/a...nces.pdf

OManuel
http://myprofile....anuelo09
rubberman
2 / 5 (3) Oct 05, 2011
Considering the mass of all the objects in the Kuiper belt/Oort cloud is more than that of all the planets/asteroids in the solar system. I imagine there will be no end of neat stuff found there.....
Neutron repulsively speaking of course...
thematrix606
1 / 5 (1) Oct 11, 2011
There's something VERY familiar about a 'spinning hourglass.'
May I be the first to suggest the informal name "Microsoft?"


I had to vote you lower cause you stole my idea! ARG :)