Noblesville meteorite, Hamilton County, Indiana, USAi
| Regional Level Types | |
|---|---|
| Noblesville meteorite | Meteorite Fall Location |
| Hamilton County | County |
| Indiana | State |
| USA | Country |
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Latitude & Longitude (WGS84):
40° 5' 7'' North , 86° 3' 18'' West
Latitude & Longitude (decimal):
Meteorite Class:
Meteoritical Society Class:
Köppen climate type:
Nearest Settlements:
| Place | Population | Distance |
|---|---|---|
| Cicero | 4,891 (2017) | 5.6km |
| Noblesville | 59,093 (2017) | 5.9km |
| Westfield | 36,738 (2017) | 7.8km |
| Arcadia | 1,666 (2017) | 10.5km |
| Carmel | 88,713 (2017) | 13.0km |
Nearest Clubs:
Local clubs are the best way to get access to collecting localities
Local clubs are the best way to get access to collecting localities
| Club | Location | Distance |
|---|---|---|
| 500 Earth Sciences Club | Indianapolis, Indiana | 36km |
Ordinary chondrite, regolith breccia (H4-6,br; S1-S2)
Fell, 31 August 1991; 484 g, one stone
Two young boys were standing outside when a whirring stone passed over them and landed with a thud ~1.3 m away and created a small 9 cm wide, 4 cm deep hole. The meteorite, covered with a nearly intact fusion-crust, was an oddly oriented wedge-shaped stone (9 cm long x 7 cm wide, base ≤ 5 cm wide) with piezoglyphs on one side of the 'wedge'. Once identified, the meteorite attracted immediate scientific attention as it consists of a number of light-colored clasts within a darker matrix. The host matrix is classified as a type H4 meteoritic assemblage with incompletely equilibrated olivine (Fa16-21) and Ca-poor pyroxene (Fs7-23±3) while the clasts are dominated by more equilibrated olivine (Fa20) and orthopyroxene (Fs18-20). Both matrix and clasts are grossly similar in overall chemistry as the dominant olivine and pyroxene (~60-70 vol%) are accompanied by subequal amounts of plagioclase, Fe-Ni metal, and troilite. Fe-Ni metal is apparently mostly kamacite (Ni 4-7 wt%), but pertinent mineralogically definitive observations are missing from the cited sources. Accessory chromite is also reported. Most intriguing, the incompletely equilibrated host material appears to be only lightly shocked, while the more equilibrated light colored H6 clasts have been shocked to shock stage S2. This suggests that the H6 material was more highly shocked and reequilibrated during some previous era before impact(s) brought it to the surface of an H4-bearing meteoroid and, later, the joint assemblage eventually encountered the earth.
Noblesville is unusually rich in solar-wind noble gases suggesting a long surface exposure for the pre-impact meteoroid. Its reported cosmic ray exposure age of ~44 Ma is significantly older than that of most H chondrites, including other H chondrite regolith breccias. As of early 2016 only 2 witnessed meteorite falls had been listed exactly as 'H4-6' meteorites [i.e., an H4, H6 mixture] with the Meteoritical Bulletin Database. It seems evident that Noblesville has had a peculiar history during its long journey from its ancestral asteroidal home(s) to a small rock on an Indiana lawn.
13 meteorites, including 4 witnessed chondrite falls are listed as confirmed meteorites for Indiana. Hamlet, Harrison County, and Rochester are the other falls. However, the Lafayette (stone) meteorite, a Martian nakhlite identified after someone studied an odd stone in a geology drawer, is probably Indiana's most famous meteorite.
Select Mineral List Type
Standard Detailed Gallery Strunz Chemical ElementsMineral List
3 valid minerals.
Meteorite/Rock Types Recorded
Note: data is currently VERY limited. Please bear with us while we work towards adding this information!
Select Rock List Type
Alphabetical List Tree DiagramDetailed Mineral List:
| ⓘ Chromite Formula: Fe2+Cr3+2O4 |
| ⓘ Enstatite Formula: Mg2Si2O6 Description: Enstatite sensu strictu [En91, 93] in a few host grains. |
| ⓘ 'Fayalite-Forsterite Series' |
| ⓘ 'Glass' |
| ⓘ 'Meteoritic Iron' Description: Nickel content (4-7%) suggests that most, if not all, of the Fe-Ni metal is kamacite.
|
| ⓘ 'Orthopyroxene Subgroup' |
| ⓘ 'Plagioclase' Formula: (Na,Ca)[(Si,Al)AlSi2]O8 |
| ⓘ 'Pyroxene Group' Formula: ADSi2O6 Description: Clast Composition: Pyroxene Fs18-20, mean 19, H4-Host Composition: Pyroxene Fs 7-22, mean 17, PMD 2%. |
| ⓘ Troilite Formula: FeS Description: Troilite is heterogeneously distributed in the matrix. |
Gallery:
List of minerals arranged by Strunz 10th Edition classification
| Group 2 - Sulphides and Sulfosalts | |||
|---|---|---|---|
| ⓘ | Troilite | 2.CC.10 | FeS |
| Group 4 - Oxides and Hydroxides | |||
| ⓘ | Chromite | 4.BB.05 | Fe2+Cr3+2O4 |
| Group 9 - Silicates | |||
| ⓘ | Enstatite | 9.DA.05 | Mg2Si2O6 |
| Unclassified | |||
| ⓘ | 'Fayalite-Forsterite Series' | - | |
| ⓘ | 'Plagioclase' | - | (Na,Ca)[(Si,Al)AlSi2]O8 |
| ⓘ | 'Pyroxene Group' | - | ADSi2O6 |
| ⓘ | 'Meteoritic Iron' | - | |
| ⓘ | 'Orthopyroxene Subgroup' | - | |
| ⓘ | 'Glass' | - | |
List of minerals for each chemical element
| O | Oxygen | |
|---|---|---|
| O | ⓘ Chromite | Fe2+Cr23+O4 |
| O | ⓘ Enstatite | Mg2Si2O6 |
| O | ⓘ Fayalite-Forsterite Series | |
| O | ⓘ Plagioclase | (Na,Ca)[(Si,Al)AlSi2]O8 |
| O | ⓘ Pyroxene Group | ADSi2O6 |
| Na | Sodium | |
| Na | ⓘ Plagioclase | (Na,Ca)[(Si,Al)AlSi2]O8 |
| Mg | Magnesium | |
| Mg | ⓘ Enstatite | Mg2Si2O6 |
| Mg | ⓘ Fayalite-Forsterite Series | |
| Al | Aluminium | |
| Al | ⓘ Plagioclase | (Na,Ca)[(Si,Al)AlSi2]O8 |
| Si | Silicon | |
| Si | ⓘ Enstatite | Mg2Si2O6 |
| Si | ⓘ Fayalite-Forsterite Series | |
| Si | ⓘ Plagioclase | (Na,Ca)[(Si,Al)AlSi2]O8 |
| Si | ⓘ Pyroxene Group | ADSi2O6 |
| S | Sulfur | |
| S | ⓘ Troilite | FeS |
| Ca | Calcium | |
| Ca | ⓘ Plagioclase | (Na,Ca)[(Si,Al)AlSi2]O8 |
| Cr | Chromium | |
| Cr | ⓘ Chromite | Fe2+Cr23+O4 |
| Fe | Iron | |
| Fe | ⓘ Chromite | Fe2+Cr23+O4 |
| Fe | ⓘ Troilite | FeS |
| Fe | ⓘ Fayalite-Forsterite Series | |
Other Regions, Features and Areas containing this locality
North AmericaContinent
North America PlateTectonic Plate
- Granite-Rhyolite ProvinceMagmatic Province
- Shawnee DomainDomain
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