These are photographs representing many of the species I have collected over the years. I have 629 species, 373 genera of brachiopods in my collection.
Pseudoatrypa decorated with manganese oxides from the Speed Quarry, Clark Co., Indiana.
These pages illustrate a lot of different kinds of fossils. Within 60 minutes of the Louisville, Kentucky, area, geological time periods represented include: Upper Ordovician, Silurian, Middle – Upper Devonian, and Mississippian (Lower Carboniferous). The Pennsylvanian (Upper Carboniferous) is a bit beyond. The Pleistocene is represented by sand & gravel, loess and cave deposits.
Consider all guides to be “works in-progress. Images and information will be added.
Cambrictites greenei – a small pyritized goniatite from the Mississippian Coral Ridge fauna of Jefferson Co., KY. Goniatites are ammonoids with undulating sutures.
I’ve collected or traded for a lot of miscellaneous fossils that aren’t diverse enough to list by category. These include fossil plants, vertebrates (mostly fish bone pieces from local bone beds), worms, graptolites, and problematic fossils that may belong to other phyla but are odd examples.
Photos – See each category
Annularia galoides in an ironstone nodule from northern Illinois.
Preservation Key : C = Calcified, Ph = Phosphatic, P = Pyritized, S = Silicified, 1= w/o, matrix, 2 = w/
Trilobites and crustaceans are arthropods, the group that includes arachnids, horseshoe crabs, millipedes, and the like. Arthropods molt as they grow. The result is common fragments and rarer complete animals. (Updated Feb. 10, 2022)
Photos of Trilobites and Other arthropods
Calymene breviceps Hall from the Waldron Shale of Clark Co., Indiana.
TRILOBITES Period Location Preservation
p = pygidium, t = thorax, c = cephalon
Arctinurus occidentalis (Hall) – Waldron Shale, Middle Silurian, Clark Co., IN – C,2
Arctinurus occidentalis (Hall) pygidium resembles a palmetto leaf
Bumastus sp. – Laurel Formation, Middle Silurian, Bardstown, Nelson Co., KY – C,2
Bumastus pygidium, a steinkern encrusted with sphalerite crystals
Calymene breviceps Hall – Waldron Shale, Middle Silurian, Clark Co., IN – C,2
Calymene breviceps Hall with pyrite – this was found attached to the floor of the Atkin’s Quarry
Cheirurus dilatatus Raymond – Waldron Shale, Middle Silurian, Clark Co., IN – C,2
Cheirurus dilatatus Raymond has a spiny pygidiumCheirurus dilatatus (Raymond) has a large glabella
Cryptolithus bellulus Ulrich – a blind trilobite from the Kope Formation, Upper Ordovician, Carrol Co., KY – C,1,2
Cryptolithus bellulus Ulrich – cephalon interior with genial spines
Eldridgeops sp. (was Phacops) – Sellersburg Limestone, Givetian, Middle Devonian, Clark Co., IN – S,1,2
Eldridgeops sp. – complete, flat and made of quartzEldridgeops sp. – front of molted cephalon on trace fossil showing compound eyes (chert replacement)
Trace fossils are evidence of action by living creatures. Examples include locomotion, feeding, nesting, excretions, etc. The division of paleontology that studies trace fossils is called “ichnology.”
Mollusks are the most abundant “shell” on a beach or riverbank. Modern cephalopods include squid, octopus and nautiloids. They are (and have always been) strictly marine. Gastropods (snails) live in the greatest diversity of ecosystems – marine, fresh & brackish water and on land. Clams are similar except for land. Monoplacophorans & scaphopods are exclusively marine. Rostroconchs are the only extinct class of mollusks.
Mollusk Photos (organized by class)
Bembexia sulcomarginata (Hall) – an exceptional specimen of a common Devonian species.
Preservation: C = Calcified, Ph = Phosphatic, P = Pyritized, S = Silicified, 1= w/o, matrix, 2 = w/ matrix
CEPHALOPODS Period Location Preservation
NAUTILOIDS
Dawsonoceras amycus Middle Silurian IN C,2
Michelinoceras sp. is generally found in small segments. This is the largest I found.
Michelinoceras sp. – Coral Ridge Member, New Providence Shale, basal Middle Mississippian, Jefferson Co., KY – P,1
Ovoceras oviforme (or Acleistoceras?) – Sellersburg = North Vernon Limestone, Clark Co., Indiana – S,1
Small, somewhat egg-shaped nautiloid
Treptoceras duseri (Hall & Whitfield) – Ubiquitous in the Upper Ordovician of the Tri-state area (IN, KY, OH), C,1,2
To be determined – large Devonian coiled nautiloid. Extremely rare, this specimen was found at the Speed Quarry in the Jeffersonville Limestone, Middle Devonian.
Large Devonian nautiloid
GONIATITES
Cantabricanites greenei (Miller) – Coral Ridge Member, New Providence Shale, basal Middle Mississippian, Jefferson Co., KY – P,1
Cantabricanites greenei (Miller) range from a few millimeters to a centimeter wide.
Polaricyclus ballardensis (Work & Mason) – Coral Ridge Member, New Providence Shale, basal Middle Mississippian, Jefferson Co., KY – P,1
Polaricyclus conkini (Work & Mason) – Coral Ridge Member, New Providence Shale, basal Middle Mississippian, Jefferson Co., KY – P,1
AMMONITES & BELEMNITES
Actinocamex verus (1) Cretaceous United Kingdom C,1
Baculites sp. Cretaceous Texas C,1
Belemitella americanus Jurassic Wyoming C,1
Hastites sp. (baculites) Lias, Early Jurassic Portugal C,1
Hildoceras bifrons ” ” ” Portugal C,1
Unidentified ” ” ” Portugal P,1
GASTROPODS/MONOPLACOPHORANS Period Location Preservation
Bellerophon gibsoni Middle Mississippian KY C,1
Bembexia sulcomarginata Middle Devonian IN S,1,2
Cyclonema sp. Upper Ordovician IN, KY C,1,2
Crytolites carinatus (Monoplacophoran) Upper Ordovician KY C,1
Glabrocingulum ellenae (Conkin), Coral Ridge Member, New Providence Shale, basal Middle Mississippian, Jefferson Co., KY – P,1 (type locality)
Glabrocingulum ellenae (Conkin) is a common pyrite-replaced snail
Globularia umbilica Upper Cretaceous MS C,1
Liospira macula Upper Ordovician KY C,1,2
Lophospira medialis Middle Ordovician KY S1,2
Lophospira biseriatus? Upper Ordovician KY C,1,2
Loxonema sp. Middle Ordovician KY S,1,2
Loxonema sp. – Coral Ridge Member, New Providence Shale, basal Middle Mississippian, Jefferson Co., KY – P,1
Loxonema sp. often shows fine growth lines
Paupospira bowdeni Upper Ordovician KY C,1,2
Natica tigra (1) Miocene Poland C,1
Naticonema lineata Middle Devonian IN C,1
Platyceras (Orthonychia) acutirostre Middle Mississippian KY C,1,2
Echinoderms are a phylum of marine animals that include sea stars, urchins, sand dollars, and the like. They are an ancient group going back to the Cambrian if not the Ediacaran. A number of classes existed for a short geological interval before going extinct. The most common echinoderm fossils in my region are crinoids and blastoids.
I’ve been involved in research in Middle Mississippian crinoids with Dr. William Ausich and Dr. Thomas Kammer. I will eventually post that research and photos of specimens. Most of the important ones were donated to the Smithsonian (U.S. National Museum) and the Orton Geological Museum at The Ohio State University.
Echinoderm Photos (organized by class – Crinozoa, Blastozoa, etc.)
Talarocrinus patei Miller & Gurley mass mortality collected by me from Sample, Kentucky
Euryocrinus veryi – top view, originally pyrite, now “limonite” (goethite) which is more stable.Euryocrinus veryi – bottom view
Euryocrinus veryi Ausich & Meyer # – from the pyritized Coral Ridge fauna, basal New Providence Shale, considered early or mid-Mississippian depending on reference. KY, IN? – Goethite,1
Granatocrinus kentuckyensis – side viewGranatocrinus kentuckyensis – top view
Granatocrinus kentuckyensis (Conkin)# – from the pyritized Coral Ridge fauna, basal New Providence Shale, considered early or mid-Mississippian depending on reference. KY, IN? – P,1
Hadroblastus sp., – side viewHadroblastus sp., – upper view
Hadroblastus sp., [H. kentuckyensis (Shumard)?] – same data as Granatocrinus kentuckyensis, though extremely rare instead of very rare. KY, IN? – P,1 Coral Ridge fauna article will be posted under articles… eventually.
Fragments of Metablastus from the Muldraugh Fm. in Hardin Co., Kentucky
Metablastus sp. # – rare, Middle Mississippian, KY – C,2
Pentremites is restricted to the Mississippian Period, primarily in North America. There are dozens of names in Galloway & Kaska’s monograph Genus Pentremites and its Species (1957). However, Dr. Alan Horowitz considered them to be overly split and that most were variations on a hand full of species.
Pentremites buttsi
Pentremites buttsi Ulrich?# – rare, Indian Springs Shale Mbr., Big Clifty Fm., Upper Mississippian, Crawford Co., Indiana.
Pentremites conoideus is an index fossil for the Salem Ls.
Pentremites conoideus Hall – Salem Ls., Middle Mississippian, IN,KY – C,1,2
Pentremites godoni (Defrance) – Upper Mississippian formations, IL,KY – C,S,1,2 This species has been further sub-divided. Two examples below.
Subspecies: Pentremites godoni pinguis Hambach (L) & abbreviatus Ulrich (R), Renault Fm. near Shetlerville, IllinoisSubspecies Pentremites godoni major, Renault Fm., Hastie Quarry, Hardin Co., IllinoisPentremites ovoides
Pentremites ovoides Ulrich# – Ste. Genevieve Ls., Mississippian, Hastie’s Quarry, Cave in Rock, Illinois. Collected ~1987, at the Oxford-West Morrison cut that no longer exists.
A deformed Pentremites patei from the Sulphur road cut, Crawford Co., Indiana
Pentremites patei Ulrich# – Indian Springs Shale Mbr., Big Clifty Fm., Upper Mississippian, Crawford Co., Indiana.
Pentremites platybasis
Pentremites platybasis Weller# – Indian Springs Shale Mbr., Big Clifty Fm., Upper Mississippian, Crawford Co., Indiana
Pentremites pulchellus
Pentremites pulchellus Ulrich# – Renault Fm., Upper Mississippian, Shetlerville, Illinois
Pentremites pyramidatus
Pentremites pyramidatus Ulrich# – Renault Fm., Upper Mississippian, Shetlerville, Illinois
Pentremites pyriformis should be the Kentucky state fossil instead of the brachiopod
Pentremites pyriformis Say – Upper Mississippian formations, IN,KY – C,1,2
Pentremites robustus – a large species
Pentremites robustus Lyon# – Glen Dean Fm?, Upper Mississippian, Madison Co., Kentucky
Pentremites springeri
Pentremites springeri Ulrich# – Indian Springs Shale Mbr., Big Clifty Fm., Upper Mississippian, Crawford Co., Indiana IN,KY
Pentremites symmetricus
Pentremites symmetricus Hall – Upper Mississippian formations, IL, IN, KY – C,S,1,2
Pentremites welleri growth series
Pentremites welleri Ulrich – Indian Springs Shale Mbr., Big Clifty Fm., Upper Mississippian, Crawford Co., Indiana
Pentremites growth series available
Tricoelocrinus woodmani – large, slightly compressed. Prepped by Tom Johnson.
Tricoelocrinus woodmani (Meek & Worthen)# – extremely rare, this specimen found on the family farm near Lanesville, Indiana, shortly before it was sold. Salem Ls. (Somerset Shale Mbr.), Middle Mississippian, IN, KY – C,1
Troosticrinus reinwardi
Troosticrinus reinwardi (Troost)# – from the Waldron Shale, Middle Silurian, in Tennessee. Similar to Decaschisma.
Comments about Pentremites
It’s possible to find more than the theca (body) and other features – including brachioles (feeding “bristles”), internal hydrospire folds (part of the respiratory system), and growth defects. No specimens like these are available for sale. Here are some examples:
Two Pentremites with columns and brachioles. Crawford Co., Indiana.3 cm view – embryonic Pentremites from holdfast to brachiolesEmbryonic Pentremites with brachioles
Perhaps the smallest complete embryonic Pentremites ever found. It will be featured in an upcoming monograph on blastoids written by the world’s experts. Found at the Sulphur exit road cut, Crawford Co., IN. Indian Springs Member of the Big Clifty Formation, Chesterian, Upper Mississippian.
Hydrospire folds on this interior of Pentremites conoideus.Hydrospire folds on this interior of Pentremites welleriHydrospire folds on this interior of Pentremites from Sulphur, Crawford Co., IndianaDeformed Pentremites welleri from Sulphur, Indiana.Deformed Pentremites symmetricus with lump near base. Sulfur, Indiana.
Photographing Echinoderms
The simplest technique is to get them wet. The problem is that they reflect light. Compare these Pentremites platybasis below.
Bryozoans appear in the fossil record in the Lower Ordovician but might be found in Late Cambrian. They are colonial animals, dominantly marine. (Freshwater species have an organic skeleton that doesn’t preserve in the fossil record.) Bryozoans are difficult to identify because the internal structure is used. However, some bryozoans have distinctive exterior features.
Septopora subquadrans Ulrich
Bryozoan Photos (more to be added)
Archimedes is the central axis of a fenestrate bryozoan. Specimens are often found in matrix.
Preservation: C = Calcified, Ph = Phosphatic, P = Pyritized, S =Silicified, 1= w/o, matrix, 2 = w/ matrix
Archimedes confertus Ulrich – Glen Dean Fm., Upper Mississippian, KY – C,1,2
Archimedes distans Ulrich central axis
Archimedes distans Ulrich – Glen Dean Fm., Upper Mississippian, KY – C,1,2
Archimedes intermedius Ulrich
Archimedes intermedius Ulrich – Glen Dean Fm., Upper Mississippian, KY – C,1,2
Archimedes invaginatus Ulrich central axis
Archimedes invaginatus Ulrich – Glen Dean Fm., Upper Mississippian, KY – C,1,2
Archimedes laxus ” ” KY C,1
Archimedes macfarlani ” ” KY C,1,2
Archimedes meekanoides McFarlan central axis
Archimedes meekanoides McFarlan – Glen Dean Fm., Upper Mississippian, KY – C,1,2
Archimedes meekanus Hall central axis
Archimedes meekanus Hall – Glen Dean Fm., Upper Mississippian, KY – C,1,2
Archimedes proutanus Ulrich central axis
Archimedes proutanus Ulrich – Glen Dean Fm., Upper Mississippian, KY – C,1,2
Archimedes sp. ” ” IN,AL C,1,2
Aspidopora newberryi (Nicholson) – about 5 mm wide
Aspidopora newberryi (Nicholson)# – a small encrusting species, Upper Ordovician, IN, KY – C1,2
Batostoma gracilis Upper Ordovician KY,IN C,1
Batostoma jamesi ” ” KY C,1
Batostoma varians ” ” KY,IN C,1
“Chaetetes” consimilis Hall
“Chaetetes” consimilis Hall# – current name unknown, flattened fronds. Waldron Shale, Silurian, IN – C,2
Cheilotrypa hispida Ulrich – 3 cm field
Cheilotrypa hispida Ulrich – very small branching bryozoan, Glen Dean Fm., Upper Mississippian, KY – C,1,2
Chondaulus ponderosa (Rominger)
Chondaulus ponderosa (Rominger) – a massive species in the Jeffersonville Ls., Middle Devonian, IN, KY – C,1,2
Constellaria florida Ulrich
Constellaria florida Ulrich – with star-shaped monticules, this genus is very distinctive. Occurs most frequently in flat fronds. Six species in the Upper Ordovician, IN, KY – C,1,2
Cyphotrypa clarksvillensis McFarlan
Cyphotrypa clarksvillensis McFarlan# – a massive, often hemispherical trepostome bryozoan of the Upper Ordovician, IN, KY – C,1
This is the version submitted and doesn’t include their editing.
By Alan Goldstein
The night sky is riddled with galaxies – vast agglomerations of stars, dust and gas. While a few seem isolated, most are found in groups or clusters containing dozens to more than a thousand galaxies. The size of an individual galaxy varies from several million stars stretching a couple thousand light years in space to more than a trillion stars spanning several hundred thousand light years.
A lot of empty space seems to lie between galaxies, but this is deceiving. Two near equal-mass galaxies several million light years apart may be drawn together by their mutual gravitational attraction. The effect both builds and destroys galaxies. These galactic collisions can be spectacular hurling stars millions of light years into intergalactic space or they can go virtually unnoticed.
Images from the Hubble telescope’s deep survey’s show that the farther back in time (more distant) one sees, the more galactic crashes may be observed. Astronomers believe (in part from these observations) that the galaxies you can see in your telescope were made by the collision and absorption of others. Physical laws favor the bigger galaxies when they smash together. Unlike a freight train hitting a compact car where the pieces scatter from the impact, the end result between galaxies can be a celestial object of amazing beauty! M51, the Whirlpool galaxy, is a classic example (photo).
M51, Whirlpool Galaxy – photo by Ron Yates
The affects of fly-bys, grazes or mergers between galaxies can make for breath-taking photography and very interesting visual observations. Watching galaxies collide is akin to seeing nature’s finest drama with a single still frame image. It would take thousands of lifetimes to see any changes between interacting galaxies. Disappointed? Don’t be – there is plenty of action “out there” and almost every combination of interaction can be observed.
“Near Misses – Near Hits?”
The gravitational influence between passing galaxies can be incredible even when they don’t appear to be in direct contact. Studies show that most galaxies are surrounded by a halo of gas and dark matter that adds to their bulk. As a result, even a “near miss” can alter the shape of one or both galaxies.
Andromeda’s M31 and M32 are the easiest pair of interacting galaxies to observe. The large spiral seems to be little affected by the proximity of dwarf elliptical M32, but in time the small galaxy will suffer. The bright compact elliptical is visible within the overall glow of the disk of M31. It is a good target for telescopes of any aperture!
M31 with M32 (9 o’clock position and M110 below – Ron Yates photo.
NGC2207 and IC2163 is a pair of spiral galaxies in Canis Major that are passing by one another. The result is a dramatic photograph – one of the favorites from the Hubble Telescope. Visually NGC2207 appears evenly illuminated and somewhat oval, while IC2163 is an open spiral with a low surface brightness giving it a ghostly appearance in comparison. Both are bright and relatively easy in a modest scope under good skies. In larger scopes a compact nucleus is visible on IC2163.
NGC4618 is an SBc barred spiral interacting with the spiral NGC4625 in Canes Venatici. The latter appears to be a compact spiral, but in reality it has a large disk that has a very low surface brightness. The smaller galaxy turns out to be is physically larger! In his 1966 publication on peculiar galaxies, H. C. Arp noted this duo as odd because the interaction created a pair of one-armed spirals! The interaction has caused both to undergo intense star formation. Both are visible with an 8-inch scope, with NGC4618 dominating the scene.
The widely spaced double system of NGC5963 and NGC5964 are Sb spiral and SO (lenticular-type) galaxies. The latter was originally described as an elliptical galaxy with unusual gas and dust clouds. Located in Virgo, they are separated by 14’ in declination. NGC5964 appears to be relatively unfazed by the proximity of NGC5963. However the latter has open spiral arms. Both are bright and are good targets for small telescopes. The SO-galaxy is an oval glow, while the spiral is smaller because the arms have a low surface brightness and require a larger scope to be well seen.
Fly-By-Night
Galaxies that are in physical contact, but do not appear to be in head-on collisions are a category I call “fly-by-night.” These graze pass one another with the outer rims of both interacting, but the main bodies remain intact. The smallest of the pair is usually “much worse for wear.” Eventually they will merge, but at the moment both galaxies are largely intact.
NGC3226 and NGC3227 is an easy target in Leo located a degree east of Gamma Leonis. At 11.4 and 10.3 magnitude, respectively, this pair is an elliptical and spiral galaxy. Their proximity has not distorted either appreciably, though deep photos show their halo stars are affected. With NGC3227 you should notice a bright stellar nucleus. It is a Seyfert galaxy with an explosive core powered by a super-massive black hole. This pair is relatively easy in a 6” and more impressive with increased aperture.
Canes Venatici is a small constellation but is well endowed with colliding galaxies. M51 is not only the favorite of the spring sky, but probably among any observer in the northern hemisphere. Called the Whirlpool Galaxy because of its easy-to-see spiral arms, it rates as the most famous interacting galaxy pair in the sky. NGC5194 and its dusty peculiar companion NGC5195 are 8.4 and 9.6 magnitude, respectively. Visible in binoculars, a 2.4” cm optical system will show it well. In moderate scopes the sweeping spiral structure may be seen and in instruments 12” and above, it can resemble its photograph.
If not overshadowed by the Whirlpool, NGC4485-90 could be the best-known colliding in Canes Venatici. It is a pair of Magellanic-type galaxies showing the slightest hints of spiral structure in good photos. The larger system NGC4490 (recently named the “Cocoon galaxy”) has a condensed nuclear region. Like the pair of NGC4618 and 25 above, this pair also shows dramatic star forming regions – only this time it is on the facing sides of each galaxy. Both are easy targets for a small telescope and are among the easiest interacting galaxies to find – less than a degree northwest of Beta Canum Venaticorium.
Impact!
When galaxies hit hard, the result can be a real galactic mess! Spiral galaxies can become so distorted and tangled that two become one. A number of galaxies at first glance do look like one weird galaxy. The advent of HST and the super-large telescopes have sufficient resolution to bring a murky mess into sharp focus.
NGC4038 and NGC4039 – the Ringtail or Antennae galaxies – are a pair of spiral galaxies with “full contact.” The “ringtail” name comes from the shape of NGC4039 with a bright ring of stars in the outer periphery and the tail is the far-flung arms of NGC4038. The “antennae” name comes from the fact that the interaction has flung stars in a pair of slightly curved arcs many times the diameter of both galaxies into deep space. The larger NGC4039 was originally type Sb. NGC4038 is a small two-armed Sc spiral. The collision has energized star-forming nebula on the facing sides and thrown dust arcing between them. In a telescope the unusual shape is easily seem in a small telescope. Look at it carefully – what shape do you see?
NGC4676A and B – the Mice – is a pair of galaxies undergoing collision and major deformation. This is a faint target at 13th magnitude, visible in telescopes larger than 8”. “A” is an SBb-type, while “B” could be an edge spiral, but is difficult to discern even with the best images because of debris from “A” crossing its middle.
NGC5128 is another very bright, very peculiar galaxy – the merging spiral and giant elliptical galaxy. The pair has become one, but the dust of the spiral bisects the globe-shaped elliptical. Also designated radio source Centaurus A, this is probably the nearest major collision at 30 million light years distant. The dust belt bisecting what would otherwise appear to be a circular elliptical type galaxy is very dramatic.
There are many other bright colliding galaxies to be observed. A second list of ten galaxies can be found on Astronomy.com. Get out and enjoy the universe’s demolition derby and enjoy the spectacle unfold in the slowest of slow motions.
Data for Selected Targets
Name Coordinates (for brightest) Mag.Vis. Size (minutes arc)