If you don't understand what to do then go to a body shop. 30 seconds to fix and adjust to the center. I had a god awful squeak/creaking sound in the cold and it was the front passenger door resting heavy on that body loop. Once you are happy tighten the bolts up firm then drive away and test. Keep the front and rear of the loop at the same height IE straight along a center line drawn horizontally through the center of the latch mechanism. Then snug the bolts just tight enough to be able to hold the door latched but loose enough to adjust by tapping with a hammer as that is where the fine tuning comes in. Once that is aligned (you may have to revisit later for tweaks) then install the body loop so that it aligns with the center of the door latch IE the lock mechanism. That stops the door from jumping up and down over bumps. Set the lower guide first so that it is snug and lines up with the door when you press it closed. If your door fits correctly then take off the looped latch completely. Please register or login to enable Dark Mode.Archived - Jeep XJ Cherokee & Grand Cherokees.Gladiator Electrical, Lighting & Sound Systems.JK Electrical, Lighting & Sound Systems.VENGEANCE - The Curmudgeons Revenge JK Build.Sponsoring Manufacturers/Vendors - Check out Cyber Monday Specials!!.JK-Forum Rules & Sponsorship Information.Those include irregular galaxies which have odd shapes, dwarf galaxies which are very small, and giant elliptical galaxies which are very large elliptical galaxies residing in the centers of some clusters of galaxies. Hubble found that some galaxies are difficult to put in the context of the tuning fork diagram. 'S0,' or lenticular galaxies, are in the transition zones between ellipticals and spirals and bridge these two types. An 'SBc' is thus a loosely wound barred spiral galaxy. Most of them feature three separate anchor points, with each anchor point occurring on a raised ridge. Continuous footman loops, however, feature multiple anchor points. They are still used to attach ropes and chains. Barred spirals have a 'B' in their classification. Continuous footman loops offer a versatile alternative to traditional, standard footman loops. The spiral arms in barred spirals usually start at the end of the bar instead of from the bulge. The most important difference between these two groups is the bar of stars that runs through the central bulge in barred spirals. In fact the spiral galaxies are sub-divided into two groups - normal spirals and barred spirals. There are indications pointing to a very close connection between the bulges of certain galaxies (Hubble types 'S0', 'Sa' and 'Sb') and elliptical galaxies. Also it is worth noting that the sizes of the round central regions in spirals - the so-called bulges - increase in size the more tightly the spiral arms are wound.

'Sa' spirals, for example, are tightly wound whereas 'Sc' spirals are more loosely wound. The spirals were assigned letters from 'a' to 'c,' which characterize the compactness of their spiral arms. Hubble gave the ellipticals numbers from zero to seven, which characterize the ellipticity of the galaxy - 'E0' is almost round, 'E7' is very elliptical. The diagram is roughly divided into two parts: elliptical galaxies (ellipticals) and spiral galaxies (spirals).

Although this scheme, also known as the Hubble tuning fork diagram, is now considered somewhat too simple, the basic ideas still hold. As one of the first steps towards a coherent theory of galaxy evolution, the American astronomer Edwin Hubble, developed a classification scheme of galaxies in 1926. Some are simple, while others are very complex in structure. Galaxies are very important fundamental building blocks of the Universe.

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