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Owners of the BMW 3 Series (E46 models) have been reporting cracks and damage in the rear subframe area of their vehicles. The issue was also common on the earlier 3 Series models and unfortunately, have reoccurred with the E46 from 1999-2006. This issue specifically appears in the rear mounting points of the subframe, which can tear out from their position in the sheet metal. This occurs as the rear differential transmits the torsional load from the engine through the subframe, and then, into the chassis of the vehicle. This constant abuse leads to fatigue in the metal, causing cracks and separation from the chassis.
The parts used for this repair includes:
Active Autowerke (www.activeautowerke.com):
• E46 Subframe / Rear Chassis Reinforcement Kit
Powerflex USA (powerflexusa.com):
• BMW E46 M3 Rear Subframe Front Bushing - Street
• BMW E46 M3 Rear Subframe Rear Bushing - Street
• BMW E46 M3 Rear Diff Rear Mount - Street
• BMW E46 M3 Rear Diff Front Mount - Street
My wife's daily driver of seven years was recently diagnosed with a rusted subframe. It was a repair that we could have afforded, but at almost fifteen years old--and also having spent almost all of that time (we presume) in the midwest--the entire car is slowly turning to rust and it is not worth our time to get it repaired.
We had decided that we would try and sell the car on Craigslist, so we spent some time cleaning the car and getting it ready. Today was going to be the final push, getting it washed and taking photos of it and making up a listing. We washed the car at home, then decided to take it to Marathon to vacuum it out before finding a parking lot to take photos in. Even from the house to the gas station, the car was acting incredibly janky, and by the time we got it to our chosen parking lot and started taking photos of it, it wasn't long before we gave up--and decided to junk the car.
We drove it home and called Victory Auto Wreckers, who will be coming to tow it away tomorrow. Here are some photos of the beloved Cavalier for posterity's sake.
"Fitting the cab, grille and wiring to the subframe"
This issue is an important stage in the assembly process as the cab is fitted to the subframe. The first part of the lower deck flooring is also supplied.
Although the front part of the lower deck floor was supplied with this issue, it is not yet fitted to the bus. This overhead view shows it in place, but not screwed down. The 30cm ruler gives an idea of size!
The submarine USS Torsk (SS-423) is credited with sinking the last enemy vessel in WWII. It went on to serve the U.S. Navy until 1968. It is now part of the Baltimore Maritime Museum and can be toured for a nominal fee... but watch your head in there... it's pretty tight!
This pretty beast came to us for a RWE APR custom front splitter, Mishimoto electric fan install, Castro motorsport 4point roll bar install & Mason Engineering rear 4point strut/subframe reinforcement, cornerbalance, allignment, and basic maintenance. Here is a list of all the current mods:
-Apex Arc-8 18x9.5 et35
-Bimmerworld Race Exhaust & Rear Diffuser
-Castro Motorsport 4point roll bar
-Custom Long Tube Headers
-Evolve Tune (custom)
--K&N Filter
-Mason Engineering Rear 4point strut/subframe reinforcement
-Mishimoto Electric Fan
-Macht Schnell Intake Elbow
-Nitto NTO5 265/35/18
-RaceWerkz APR Front Splitter (custom)
-Status Gruppe CSL Front Bumper, CSL Race Lip, CSL Trunk, Section 1 Resonated, and Coilover Kit.
Owners of the BMW 3 Series (E46 models) have been reporting cracks and damage in the rear subframe area of their vehicles. The issue was also common on the earlier 3 Series models and unfortunately, have reoccurred with the E46 from 1999-2006. This issue specifically appears in the rear mounting points of the subframe, which can tear out from their position in the sheet metal. This occurs as the rear differential transmits the torsional load from the engine through the subframe, and then, into the chassis of the vehicle. This constant abuse leads to fatigue in the metal, causing cracks and separation from the chassis.
The parts used for this repair includes:
Active Autowerke (www.activeautowerke.com):
• E46 Subframe / Rear Chassis Reinforcement Kit
Powerflex USA (powerflexusa.com):
• BMW E46 M3 Rear Subframe Front Bushing - Street
• BMW E46 M3 Rear Subframe Rear Bushing - Street
• BMW E46 M3 Rear Diff Rear Mount - Street
• BMW E46 M3 Rear Diff Front Mount - Street
29 May 2022, ~11pm ET, Springfield Virginia USA. Orion Atlas AZ/EQ-G Pro mount. QHY 294M Pro camera @ -10C, bin 2x2, exposure 30 seconds, gain 2600, 11MP mode, stack of 40 subframes, no calibration frames. Baader Luminance filter. Reprocessed in Siril and PS on 25 May 2023.
Clouds: partly cloudy
Seeing: avg
Transparency: avg
Moon phase: 1%
FOV: 31 x 29 arcmin.
Resolution: 0.9 arcsec/pixel.
Appearance: Loosely wound face-on spiral galaxy, pinwheel shape.
From Wikipedia:
The Pinwheel Galaxy (also known as Messier 101, M101 or NGC 5457) is a face-on spiral galaxy 21 million light-years (6.4 megaparsecs) away from Earth in the constellation Ursa Major. It was discovered by Pierre Méchain in 1781 and was communicated that year to Charles Messier, who verified its position for inclusion in the Messier Catalogue as one of its final entries.
On February 28, 2006, NASA and the European Space Agency released a very detailed image of the Pinwheel Galaxy, which was the largest and most-detailed image of a galaxy by Hubble Space Telescope at the time. The image was composed of 51 individual exposures, plus some extra ground-based photos.
On August 24, 2011, a Type Ia supernova, SN 2011fe, was discovered in M101.
Pierre Méchain, the discoverer of the galaxy, described it as a "nebula without star, very obscure and pretty large, 6' to 7' in diameter, between the left hand of Bootes and the tail of the great Bear. It is difficult to distinguish when one lits the [grating] wires."
William Herschel wrote in 1784 that the galaxy was one of several which "...in my 7-, 10-, and 20-feet [focal length] reflectors shewed a mottled kind of nebulosity, which I shall call resolvable; so that I expect my present telescope will, perhaps, render the stars visible of which I suppose them to be composed."
Lord Rosse observed the galaxy in his 72-inch-diameter Newtonian reflector during the second half of the 19th century. He was the first to make extensive note of the spiral structure and made several sketches.
To observe the spiral structure in modern instruments requires a fairly large instrument, very dark skies, and a low-power eyepiece.
M101 is a large galaxy, with a diameter of 170,000 light-years. By comparison, the Milky Way has a diameter of between 100,000 and 120,000 light-years. It has around a trillion stars. It has a disk mass on the order of 100 billion solar masses, along with a small central bulge of about 3 billion solar masses. Its characteristics can be compared to those of Andromeda Galaxy.
M101 has a high population of H II regions, many of which are very large and bright. H II regions usually accompany the enormous clouds of high density molecular hydrogen gas contracting under their own gravitational force where stars form. H II regions are ionized by large numbers of extremely bright and hot young stars; those in M101 are capable of creating hot superbubbles. In a 1990 study, 1,264 H II regions were cataloged in the galaxy. Three are prominent enough to receive New General Catalogue numbers—NGC 5461, NGC 5462, and NGC 5471.
M101 is asymmetrical due to the tidal forces from interactions with its companion galaxies. These gravitational interactions compress interstellar hydrogen gas, which then triggers strong star formation activity in M101's spiral arms that can be detected in ultraviolet images.
In 2001, the X-ray source P98, located in M101, was identified as an ultra-luminous X-ray source—a source more powerful than any single star but less powerful than a whole galaxy—using the Chandra X-ray Observatory. It received the designation M101 ULX-1. In 2005, Hubble and XMM-Newton observations showed the presence of an optical counterpart, strongly indicating that M101 ULX-1 is an X-ray binary. Further observations showed that the system deviated from expected models—the black hole is just 20 to 30 solar masses, and consumes material (including captured stellar wind) at a higher rate than theory suggests.
It is estimated that M101 has about 150 globular clusters, the same as the number of the Milky Way's globular clusters.
M101 has six prominent companion galaxies: NGC 5204, NGC 5474, NGC 5477, NGC 5585, UGC 8837 and UGC 9405. As stated above, the gravitational interaction between it and its satellites may have spawned its grand design pattern. The galaxy has probably distorted the second-listed companion.
Four internal supernovae have been recorded:
SN 1909A, was discovered by Max Wolf in January 1909 and reached magnitude 12.1. SN 1951H reached magnitude 17.5 in September 1951. SN 1970G reached magnitude 11.5 in January 1970. On August 24, 2011, a Type Ia supernova, SN 2011fe, initially designated PTF 11kly, was discovered in M101. It had visual magnitude 17.2 at discovery and reached 9.9 at its peak.
On February 10, 2015, a luminous red nova, known as M101 OT2015-1 was discovered in the Pinwheel Galaxy.
Aluminum subframe fabricated by Marin in Spain.
I took the photo at Jerez circuit during the last round of the 2008 Spanish Championship.
More info at www.bottpower.com
HONDA.Motorcycle-Blogs.info
, HONDA, CBR, CBR600RR, CBR1000RR, 600RR, 1000RR, CBR954RR, 954RR, CBR929RR, 929RR, CBR900RR, 900RR, F4i, CBR600, FIREBLADE
stores.ebay.com/Motorcycle-Center - Motorcycle Center sells oem Motorcycle Parts that fit Honda Motorcycles - oem motorcycle parts
Owners of the BMW 3 Series (E46 models) have been reporting cracks and damage in the rear subframe area of their vehicles. The issue was also common on the earlier 3 Series models and unfortunately, have reoccurred with the E46 from 1999-2006. This issue specifically appears in the rear mounting points of the subframe, which can tear out from their position in the sheet metal. This occurs as the rear differential transmits the torsional load from the engine through the subframe, and then, into the chassis of the vehicle. This constant abuse leads to fatigue in the metal, causing cracks and separation from the chassis.
The parts used for this repair includes:
Active Autowerke (www.activeautowerke.com):
• E46 Subframe / Rear Chassis Reinforcement Kit
Powerflex USA (powerflexusa.com):
• BMW E46 M3 Rear Subframe Front Bushing - Street
• BMW E46 M3 Rear Subframe Rear Bushing - Street
• BMW E46 M3 Rear Diff Rear Mount - Street
• BMW E46 M3 Rear Diff Front Mount - Street
My wife's daily driver of seven years was recently diagnosed with a rusted subframe. It was a repair that we could have afforded, but at almost fifteen years old--and also having spent almost all of that time (we presume) in the midwest--the entire car is slowly turning to rust and it is not worth our time to get it repaired.
We had decided that we would try and sell the car on Craigslist, so we spent some time cleaning the car and getting it ready. Today was going to be the final push, getting it washed and taking photos of it and making up a listing. We washed the car at home, then decided to take it to Marathon to vacuum it out before finding a parking lot to take photos in. Even from the house to the gas station, the car was acting incredibly janky, and by the time we got it to our chosen parking lot and started taking photos of it, it wasn't long before we gave up--and decided to junk the car.
We drove it home and called Victory Auto Wreckers, who will be coming to tow it away tomorrow. Here are some photos of the beloved Cavalier for posterity's sake.
Speedshop.ch Lancia Delta HF Rear Differential Steel Subframe
Option of rear Uniball Steel Trailer Radial and Longitudal.
More infos and enquiries: info@speedshop.ch
Owners of the BMW 3 Series (E46 models) have been reporting cracks and damage in the rear subframe area of their vehicles. The issue was also common on the earlier 3 Series models and unfortunately, have reoccurred with the E46 from 1999-2006. This issue specifically appears in the rear mounting points of the subframe, which can tear out from their position in the sheet metal. This occurs as the rear differential transmits the torsional load from the engine through the subframe, and then, into the chassis of the vehicle. This constant abuse leads to fatigue in the metal, causing cracks and separation from the chassis.
The parts used for this repair includes:
Active Autowerke (www.activeautowerke.com):
• E46 Subframe / Rear Chassis Reinforcement Kit
Powerflex USA (powerflexusa.com):
• BMW E46 M3 Rear Subframe Front Bushing - Street
• BMW E46 M3 Rear Subframe Rear Bushing - Street
• BMW E46 M3 Rear Diff Rear Mount - Street
• BMW E46 M3 Rear Diff Front Mount - Street
Captured 16 May 2022, ~23:00 hrs ET, Springfield, VA, USA. Bortle 8 skies, Celestron 8 inch SCT at f/6.3 (eff. fl 1290mm), Orion Atlas AZ/EQ-G Pro mount. QHY 294M Pro camera @ -10C, bin 1, exposure 32 seconds, gain 3100, 11MP mode, stack of 20 subframes, no calibration frames used. Baader Luminance filter.
Clouds: clear
Seeing: avg
Transparency: avg
Moon phase: full
FOV: 36 x 33 arcmin.
Resolution: 1.0 arcsec/pixel.
Orientation: Up is West.
Appearance: Classic globular cluster.
Notes: Focused center FOV. Unguided.
From Wikipedia:
Messier 13 or M13, also designated NGC 6205 and sometimes called the Great Globular Cluster in Hercules or the Hercules Globular Cluster, is a globular cluster of several hundred thousand stars in the constellation of Hercules.
M13 was discovered by Edmond Halley in 1714, and cataloged by Charles Messier on June 1, 1764.
About one third of the way from Vega to Arcturus, four bright stars in Hercules form the Keystone asterism, the broad torso of the hero. M13 can be seen in this asterism 2⁄3 of the way north (by west) from Zeta to Eta Herculis. Although only telescopes with great light-gathering capability fully resolve the stars of the cluster, M13 may be visible to the naked eye depending on circumstances. With a low-power telescope, Messier 13 looks like a comet or fuzzy patch. The cluster is visible throughout the year from latitudes greater than 36 degrees north, with the longest visibility during Northern Hemisphere spring and summer.
With an apparent magnitude of 5.8, it is barely visible with the naked eye on clear nights. Its diameter is about 23 arcminutes and it is readily viewable in small telescopes.
In traditional binoculars, the Hercules Globular Cluster appears as a round patch of light. At least four inches of telescope aperture resolves stars in M13's outer extent as small pinpoints of light. However, only larger telescopes resolve stars further into the center of the cluster.
About 145 light-years in diameter, M13 is composed of several hundred thousand stars, the brightest of which is a red giant, the variable star V11, also known as V1554 Herculis, with an apparent visual magnitude of 11.95. M13 is 22,200–25,000 light-years away from Earth, and the globular cluster is one of over one hundred that orbit the center of the Milky Way.
Single stars in this globular cluster were first resolved in 1779. Compared to the stars in the neighborhood of the Sun, the stars of the M13 population are more than a hundred times more densely packed. They are so close together that they sometimes collide and produce new stars. The newly formed, young stars, so-called "blue stragglers", are particularly interesting to astronomers.
The 1974 Arecibo message, which contained encoded information about the human race, DNA, atomic numbers, Earth's position and other information, was beamed from the Arecibo Observatory radio telescope towards M13 as an experiment in contacting potential extraterrestrial civilizations in the cluster. The cluster will move through space during the transit time; opinions differ as to whether or not the cluster will be in a position to receive the message by the time that it arrives.
The last two variables (V63 and V64) were discovered from Spain in April 2021 and March 2022 respectively.
Jaguar Cars Ltd., better known simply as Jaguar is a British luxury car manufacturer, headquartered in Coventry, England. It has been a wholly-owned subsidiary of the Indian company Tata Motors Ltd. since March 2008 and is operated as part of the Jaguar Land Rover business.
Jaguar was founded as the Swallow Sidecar Company by Sir William Lyons in 1922, originally making motorcycle sidecars before switching to passenger cars. The name was changed to Jaguar after World War II due to the unfavourable connotations of the SS initials.
The Jaguar D-Type, like its predecessor the C-Type, was a factory-built race car. Although it shared the basic straight-6 XK engine design (initially 3.4L and eventually uprated to 3.8 litres in the late fifties) with the C-Type, the majority of the car was radically different. Perhaps its most ground-breaking innovation was the introduction of a monocoque chassis, which not only introduced aircraft-style engineering to competition car design, but also an aeronautical understanding of aerodynamic efficiency. The D-Type was introduced purely for competition, but after Jaguar withdrew from racing, the company offered the remaining, unfinished chassis as the roadgoing Jaguar XKSS, by making changes to the racers: adding an extra seat, another door, a full-width windshield and primitive folding top, as concessions to practicality. However, on the evening of 12 February 1957, a fire broke out at the Browns Lane plant destroying nine of the twenty five cars that had already been completed or in semi-completion. Production is thought to have included 53 customer D-Types, 18 factory team cars, and 16 XKSS versions.
The new chassis followed aircraft engineering practice, being manufactured according to monocoque principles. The central tub, within which the driver sat, was formed from sheets of aluminium alloy. To this was attached an aluminium tubing subframe carrying the bonnet, engine, front suspension, and steering assembly. The rear suspension and final drive were mounted directly onto the monocoque itself. Fuel was carried in deformable bags inside cells within the monocoque; another aircraft innovation.
The highly efficient, aerodynamic bodywork was largely the work of Malcolm Sayer, who joined Jaguar following a stint with the Bristol Aeroplane Company during World War II. Although he also worked on the C-Type, the limitations of the conventional separate-chassis did not allow full expression of his talent. For the D-Type, Sayer insisted on a minimal frontal area. To reduce its height, Haynes and former-Bentley engineer Walter Hassan developed dry sump lubrication for the XK engine. By also canting the engine over by 8° (resulting in the trademark, off-centre bonnet bulge) the reduction in area was achieved. Care was taken to reduce drag due to the underbody, resulting in an unusually high top speed; for the long Mulsanne Straight at Le Mans, a large vertical stabiliser was mounted behind the driver's head for aerodynamic stability with minimum drag. For the 1955 season, factory cars were fitted with a revised, long-nose version of the bodywork, which increased top speed even further.
Mechanically, many features were shared with the outgoing C-Type. The ground-breaking disc brakes were retained, as was the XK engine. Apart from the new lubrication system, as development progressed during the D-Type's competition life the engine was also revised. 1955 saw the introduction of larger valves, and an asymmetrical cylinder head design within which to accommodate them. The Jaguar D-Type was the second racing car to have Dunlop disk brakes. The Citroën DS, introduced a year later, was the first production car with disk brakes in Europe. The Crosley Hotshot was the first American automobile with disk brakes, in 1949.