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Jagdish Dukre
OPTIC NERVE HYPOPLASIA 
Optic nerve hypoplasia (ONH) is the most common 
optic disc anomaly and is the third leading cause of 
blindness in children in the western world after 
cerebral damage and retinopathy of prematurity. 
Risk factors for ONH include 
 young maternal age, 
 maternal smoking, 
 preterm birth and its complications.
Clinical features 
 An abnormally small optic 
nerve head. 
 Double-ring sign: 
 The optic nerve is pale 
surrounded by a yellowish 
peripapillary ring of sclera and 
an outer concentric ring of 
hypopigmentation. 
 outer ring of normal junction 
between sclera and lamina 
cribrosa 
 inner ring denoting extension of 
retina and RPE over lamina 
cribrosa
A disc to centre of macula (DM): mean disc diameter 
(DD) ratio 
DM:DD ratio of 
 3.00 should lead to serious consideration of the diagnosis 
and a value of 
 4.00 probably accords a definitive diagnosis. 
 The visual acuity is associated with the DM: DD ratio. 
 In one study of 19 children with ONH, all eyes with a DM: 
DD ratio of more than 3 had reduced visual acuities but all 
those with a ratio of less than 3 had normal acuities.
Histopathologically, 
 optic nerve hypoplasia has subnormal number of 
axons with normal mesodermal elements and glial 
supporting tissue. 
 A reduction in the diameter of the hypoplastic optic 
nerve and chiasm is demonstrated reliably by MRI, 
which establishes the presumptive diagnosis of optic 
nerve hypoplasia.
Visual acuity: 
 ranges from 20/20 to no light perception. 
 Visual acuity usually remains stable throughout life unless 
amblyopia develops in one eye or it is associated with 
suprasellar tumour where it can lead to acquired visual loss. 
 Optic nerve hypoplasia has recently been implicated in the 
pathogenesis of amblyopia although it is still not clear whether 
a small optic disc area is the cause for decreased vision or the 
associated hyperopia and anisometropia.
Visual field defects: the affected eye shows localized visual 
field defects. 
Astigmatism: warrants attention to correction of refractive 
error in children. 
Associations: Magnetic resonance imaging has revealed 
coexistent CNS abnormalities with ONH. 
1) Isolated ONH: A reduction in the diameter of the 
hypoplastic optic nerve and chiasm is demonstrated reliably by 
MRI, which establishes the presumptive diagnosis of optic nerve 
hypoplasia. 
2) Septo-optic dysplasia (de Morsier syndrome) 
constellation of optic nerve hypoplasia, absence of the septum 
pellucidum, and partial or complete agenesis of the corpus 
callosum.
sagittal MR shows absence of the 
corpus callosum
3) Forebrain malformations, schizencephaly and periventricular 
leukomalacia, absence of the pituitary infundibulum with or 
without posterior pituitary ectopia (can present in upto 74%) 
 Cerebral hemispheric abnormalities indicate that 
neurodevelopmental deficits are likely. 
 Absence of the pituitary infundibulum with an ectopic 
posterior pituitary gland indicates congenital hypopituitarism 
and warrants endocrinologic evaluation in children. 
 Growth hormone deficiency is most common which usually 
presents by 3-4 yrs of age
MORNING GLORY DISC ANOMALY 
 The morning glory disc anomaly is a 
congenital excavation of posterior globe 
that involves the optic disc. 
 The term reflects the morphological 
similarity to the flower of the morning 
glory plant. 
 Morning glory syndrome is ostensibly a 
sporadic condition. 
 It usually occurs as a unilateral condition, 
though bilateral lesions have been 
reported. 
 Morning glory discs are more common in 
females (2:1)
Pathogenesis 
 The pathogenesis of the condition is unknown. 
 One hypothesis argues that the condition results from 
failure of closure of the foetal fissure and that it is a 
variant of optic nerve coloboma. 
 Alternatively, a primary mesenchymal abnormality has 
been postulated on the basis of the glial tuft, the 
scleral and vascular abnormalities.
Clinical features 
Ophthalmosopic appearance: 
It is characterized by 
funnel-shaped and enlarged 
dysplastic optic disc with 
white tissue, and retinal 
vessels arising from the 
periphery of the disc (spoke 
wheel pattern) and running 
an abnormally straight 
course over the peripapillary 
retina .
 Visual acuity: visual acuity is often very low, being in the 
range of counting fingers to 6/60, but it can be associated 
with no perception of light. 
 Amblyopia: variable depth based on the extent of the 
alteration of the nerve fiber layer and difficult to predict 
on the basis of disc appearance
Associations 
With rare exceptions, the Morning glory disc anomaly is not 
part of a multisystem genetic disorder. 
Ocular anomalies 
Retinal detachment, both serous and rhegmatogenous, occurs 
in about one- third (26-38%) cases of MGDA. 
Strabismus 
Intracranial disorders 
Basal encephalocele: Children who have this occult basal 
encephalocele have characteristic facial features including 
hypertelorism, depressed nasal bridge, midline upper lip notch 
and sometimes midline cleft in soft palate. 
Agenesis of corpus callosum 
Absence of chiasm 
Panhypopituitarism 
Most affected children have no overt intellectual or neurologic 
deficits.
(A) Morning glory optic disc anomaly; (B) hypertelorism and flat nasal 
bridge – note bilateral iris colobomas;
OPTIC DISC COLOBOMA 
 Optic disc coloboma can be present in one or both 
eyes. 
 They may arise sporadically or be inherited in 
autosomal dominant fashion. 
 It has recently been shown to be associated with PAX2 
gene mutations as part of the renal-coloboma 
syndrome. 
 Pathogenesis: It is caused by an incomplete or 
abnormal apposition of the proximal ends of the 
embryonic fissure.
Clinical features 
 Optic disc coloboma is 
typically an enlarged disc 
with sharply demarcated, 
focal, glistening bowl 
shaped excavation of the 
optic disc. 
 The coloboma occupies the 
lower part of the optic nerve 
head. 
 The neuro-retinal rim is 
absent inferiorly but is 
usually identifiable 
superiorly.
(A) Optic disc coloboma; (B) FA shows hypofluorescence of the cavity
 Visual acuity: may be minimally or severely affected 
and difficult to predict based on the appearance. 
 Careful analysis of the photographic appearances of 
colobomata involving the optic nerve has shown that 
the only feature that relates to visual outcome is the 
degree of foveal involvement by the coloboma. 
 Significant refractive error and anisometropia are 
common and need to be dealt with optimal glass 
prescription.
Associations 
Optic nerve colobomas may be associated with the 
following 
 Microphthalmos 
 Iris coloboma, lens coloboma and retinochoroidal 
coloboma 
 Serous macular detachment: can be rhegmatogenous or 
non rhegmatogenous. 
 Systemic associations like : 
 CHARGE syndrome (coloboma, heart anomaly, choanal 
atresia, retardation, genital and ear anomalies) 
 Walker-Warburg syndrome 
 Goldenhar’s syndrome
It needs to be distinguished from the other congenital disc lesions, 
especially morning glory disc .
OPTIC PIT 
 Optic nerve pits are rare congenital anomalies that are 
part of a spectrum of congenital cavitary optic disc 
anomalies that may be associated with juxtapapillary 
retinal detachments. 
 They occur in less than 1 in 10,000 patients seen in an 
ophthalmic setting and are bilateral in 10% to 15% of 
cases.
Pathogenesis 
 These are formed through the herniation of dysplastic 
retina into a collagen-lined pocket extending posteriorly 
through a defect in the lamina cribrosa. 
 They occur in locations unrelated to the embryonic 
fissure, commonly located at temporal aspect of disc
Clinical features 
 An optic disc pit is a round or 
oval, gray, white or yellowish 
depression in the optic nerve 
head. 
 Visual acuity is usually 
normal unless associated 
with serous macular 
detachment. 
 Visual field defects: 
paracentral arcuate scotoma 
is the most common.
(A) Optic disc pit; (B) optic disc pit and macular detachment
Associations 
 Approximately one third to two thirds of patients with 
optic pits develop serous macular detachments. 
 These may occur during childhood or late in life but 
are most common between the ages of 20 and 40. 
 The fluid from optic pit initially produces an inner 
layer retinal separation (retinoschisis) that overlies 
posterior pole which then develops outer macular hole 
and leads to serous macular detachment
 Various theories have been postulated for the source of 
the subretinal fluid such as 
1) cerebrospinal fluid (CSF), 
2) liquefied vitreous entering through the pit or through 
a macular hole, and 
3) leakage from either choroidal vessels or permeable 
vessels in the pit. 
 Optic pits are not associated with brain malformations 
– so they do not warrant neuroimaging.
Treatment 
The treatment of serous macular detachment associated with an 
optic disc pit is still controversial. 
 Observation: spontaneous resolution has been seen in 25% 
cases. 
 Laser photocoagulation: creating a barrier of chorioretinal 
adhesions at the temporal optic disc border but repeated 
treatments may be required. 
 Gas tamponade with laser photocoagulation: this induces 
pneumatic displacement of the outer layer detachment and 
improves central vision. 
 Pars plana vitrectomy (PPV) combined with laser 
photocoagulation and gas tamponade: currently this 
approach is considered to be more effective than laser 
photocoagulation or gas tamponade alone, particularly in eyes 
with severe visual loss
MEGALOPAPILLA 
 Megalopapilla is a generic term that connotes an 
abnormally large optic disc that lacks the inferior 
excavation of optic disc coloboma or the numerous 
anomalous features of the morning glory disc anomaly. 
 This condition is usually bilateral and often associated with 
a large cup-to-disc ratio. 
 Patients who have megalopapilla are often suspected to 
have glaucoma. 
 Unlike the situation in glaucoma, however, the optic cup is 
usually round or horizontally oval with no vertical notch or 
encroachment .
 Visual acuity is generally normal in megalopapilla but may 
be mildly decreased in some cases. 
 Visual fields are usually normal except for an enlarged blind 
spot, which enables the examiner to rule out low-tension 
glaucoma or a compressive lesion. 
 Megalopapilla is only rarely associated with brain anomalies, 
and neuroimaging is not warranted unless midline facial 
anomalies are present.
CONGENITAL TILTED DISC SYNDROME 
 The tilted disc syndrome is a nonhereditary bilateral 
condition. 
 The superotemporal optic disc is elevated and the 
inferonasal disc is displaced posteriorly, which results in 
an optic disc of oval appearance with its long axis 
obliquely orientated. 
 This configuration is accompanied by situs inversus of 
the retinal vessels, congenital inferonasal conus, 
thinning of the inferonasal retinal pigment epithelium 
and choroid, and myopic astigmatism. 
 These features presumably result from a generalized 
ectasia of the inferonasal fundus that involves the 
corresponding sector of the optic disc.
(A) Tilted disc; (B) tilted disc and inferonasal chorioretinal thinning
 Familiarity with this condition is important because 
affected patients may present with the suggestion of 
bitemporal hemianopias, which involve primarily the 
superotemporal quadrants. 
 However, these field defects, when observed carefully, do 
not respect the vertical meridian (as do chiasmal 
lesions). 
 Furthermore, large and small isopters are fairly normal, 
but medium-sized isopters are constricted selectively 
because of the ectasia of the midperipheral fundus.
 Repeated visual field tests after correcting for the myopic 
refractive error often eliminate the field defect, which 
confirms its refractive nature. 
 In some cases, retinal sensitivity is decreased in the area 
of the ectasia, which causes the defect to persist despite 
refractive correction. 
 Rare cases of the tilted disc syndrome have been 
documented in patients who have congenital suprasellar 
tumors; neuroimaging is therefore warranted when the 
associated bitemporal hemianopia respects the vertical 
meridian.
CONGENITAL OPTIC DISC PIGMENTATION 
 Congenital optic disc pigmentation is a condition in which 
melanin anterior to or within the lamina cribrosa imparts a gray 
appearance to the disc.
 True congenital optic disc pigmentation is extremely rare. 
 Congenital optic pigmentation is compatible with good 
visual acuity but may be associated with coexistent optic 
disc anomalies that decrease vision. 
 Most cases of gray optic discs are not caused by congenital 
optic disc pigmentation. 
 For reasons that are understood poorly, optic discs of 
infants who have delayed visual maturation or albinism and 
those of some normal neonates have a diffuse gray tint 
when viewed ophthalmoscopically. 
 In these disorders, the gray tint disappears within the first 
year of life without visible pigment migration.
Congenital optic disc anomalies

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Congenital optic disc anomalies

  • 2. OPTIC NERVE HYPOPLASIA Optic nerve hypoplasia (ONH) is the most common optic disc anomaly and is the third leading cause of blindness in children in the western world after cerebral damage and retinopathy of prematurity. Risk factors for ONH include  young maternal age,  maternal smoking,  preterm birth and its complications.
  • 3. Clinical features  An abnormally small optic nerve head.  Double-ring sign:  The optic nerve is pale surrounded by a yellowish peripapillary ring of sclera and an outer concentric ring of hypopigmentation.  outer ring of normal junction between sclera and lamina cribrosa  inner ring denoting extension of retina and RPE over lamina cribrosa
  • 4.
  • 5. A disc to centre of macula (DM): mean disc diameter (DD) ratio DM:DD ratio of  3.00 should lead to serious consideration of the diagnosis and a value of  4.00 probably accords a definitive diagnosis.  The visual acuity is associated with the DM: DD ratio.  In one study of 19 children with ONH, all eyes with a DM: DD ratio of more than 3 had reduced visual acuities but all those with a ratio of less than 3 had normal acuities.
  • 6. Histopathologically,  optic nerve hypoplasia has subnormal number of axons with normal mesodermal elements and glial supporting tissue.  A reduction in the diameter of the hypoplastic optic nerve and chiasm is demonstrated reliably by MRI, which establishes the presumptive diagnosis of optic nerve hypoplasia.
  • 7. Visual acuity:  ranges from 20/20 to no light perception.  Visual acuity usually remains stable throughout life unless amblyopia develops in one eye or it is associated with suprasellar tumour where it can lead to acquired visual loss.  Optic nerve hypoplasia has recently been implicated in the pathogenesis of amblyopia although it is still not clear whether a small optic disc area is the cause for decreased vision or the associated hyperopia and anisometropia.
  • 8. Visual field defects: the affected eye shows localized visual field defects. Astigmatism: warrants attention to correction of refractive error in children. Associations: Magnetic resonance imaging has revealed coexistent CNS abnormalities with ONH. 1) Isolated ONH: A reduction in the diameter of the hypoplastic optic nerve and chiasm is demonstrated reliably by MRI, which establishes the presumptive diagnosis of optic nerve hypoplasia. 2) Septo-optic dysplasia (de Morsier syndrome) constellation of optic nerve hypoplasia, absence of the septum pellucidum, and partial or complete agenesis of the corpus callosum.
  • 9. sagittal MR shows absence of the corpus callosum
  • 10. 3) Forebrain malformations, schizencephaly and periventricular leukomalacia, absence of the pituitary infundibulum with or without posterior pituitary ectopia (can present in upto 74%)  Cerebral hemispheric abnormalities indicate that neurodevelopmental deficits are likely.  Absence of the pituitary infundibulum with an ectopic posterior pituitary gland indicates congenital hypopituitarism and warrants endocrinologic evaluation in children.  Growth hormone deficiency is most common which usually presents by 3-4 yrs of age
  • 11. MORNING GLORY DISC ANOMALY  The morning glory disc anomaly is a congenital excavation of posterior globe that involves the optic disc.  The term reflects the morphological similarity to the flower of the morning glory plant.  Morning glory syndrome is ostensibly a sporadic condition.  It usually occurs as a unilateral condition, though bilateral lesions have been reported.  Morning glory discs are more common in females (2:1)
  • 12. Pathogenesis  The pathogenesis of the condition is unknown.  One hypothesis argues that the condition results from failure of closure of the foetal fissure and that it is a variant of optic nerve coloboma.  Alternatively, a primary mesenchymal abnormality has been postulated on the basis of the glial tuft, the scleral and vascular abnormalities.
  • 13. Clinical features Ophthalmosopic appearance: It is characterized by funnel-shaped and enlarged dysplastic optic disc with white tissue, and retinal vessels arising from the periphery of the disc (spoke wheel pattern) and running an abnormally straight course over the peripapillary retina .
  • 14.
  • 15.  Visual acuity: visual acuity is often very low, being in the range of counting fingers to 6/60, but it can be associated with no perception of light.  Amblyopia: variable depth based on the extent of the alteration of the nerve fiber layer and difficult to predict on the basis of disc appearance
  • 16. Associations With rare exceptions, the Morning glory disc anomaly is not part of a multisystem genetic disorder. Ocular anomalies Retinal detachment, both serous and rhegmatogenous, occurs in about one- third (26-38%) cases of MGDA. Strabismus Intracranial disorders Basal encephalocele: Children who have this occult basal encephalocele have characteristic facial features including hypertelorism, depressed nasal bridge, midline upper lip notch and sometimes midline cleft in soft palate. Agenesis of corpus callosum Absence of chiasm Panhypopituitarism Most affected children have no overt intellectual or neurologic deficits.
  • 17. (A) Morning glory optic disc anomaly; (B) hypertelorism and flat nasal bridge – note bilateral iris colobomas;
  • 18. OPTIC DISC COLOBOMA  Optic disc coloboma can be present in one or both eyes.  They may arise sporadically or be inherited in autosomal dominant fashion.  It has recently been shown to be associated with PAX2 gene mutations as part of the renal-coloboma syndrome.  Pathogenesis: It is caused by an incomplete or abnormal apposition of the proximal ends of the embryonic fissure.
  • 19. Clinical features  Optic disc coloboma is typically an enlarged disc with sharply demarcated, focal, glistening bowl shaped excavation of the optic disc.  The coloboma occupies the lower part of the optic nerve head.  The neuro-retinal rim is absent inferiorly but is usually identifiable superiorly.
  • 20. (A) Optic disc coloboma; (B) FA shows hypofluorescence of the cavity
  • 21.  Visual acuity: may be minimally or severely affected and difficult to predict based on the appearance.  Careful analysis of the photographic appearances of colobomata involving the optic nerve has shown that the only feature that relates to visual outcome is the degree of foveal involvement by the coloboma.  Significant refractive error and anisometropia are common and need to be dealt with optimal glass prescription.
  • 22. Associations Optic nerve colobomas may be associated with the following  Microphthalmos  Iris coloboma, lens coloboma and retinochoroidal coloboma  Serous macular detachment: can be rhegmatogenous or non rhegmatogenous.  Systemic associations like :  CHARGE syndrome (coloboma, heart anomaly, choanal atresia, retardation, genital and ear anomalies)  Walker-Warburg syndrome  Goldenhar’s syndrome
  • 23. It needs to be distinguished from the other congenital disc lesions, especially morning glory disc .
  • 24. OPTIC PIT  Optic nerve pits are rare congenital anomalies that are part of a spectrum of congenital cavitary optic disc anomalies that may be associated with juxtapapillary retinal detachments.  They occur in less than 1 in 10,000 patients seen in an ophthalmic setting and are bilateral in 10% to 15% of cases.
  • 25. Pathogenesis  These are formed through the herniation of dysplastic retina into a collagen-lined pocket extending posteriorly through a defect in the lamina cribrosa.  They occur in locations unrelated to the embryonic fissure, commonly located at temporal aspect of disc
  • 26. Clinical features  An optic disc pit is a round or oval, gray, white or yellowish depression in the optic nerve head.  Visual acuity is usually normal unless associated with serous macular detachment.  Visual field defects: paracentral arcuate scotoma is the most common.
  • 27. (A) Optic disc pit; (B) optic disc pit and macular detachment
  • 28. Associations  Approximately one third to two thirds of patients with optic pits develop serous macular detachments.  These may occur during childhood or late in life but are most common between the ages of 20 and 40.  The fluid from optic pit initially produces an inner layer retinal separation (retinoschisis) that overlies posterior pole which then develops outer macular hole and leads to serous macular detachment
  • 29.  Various theories have been postulated for the source of the subretinal fluid such as 1) cerebrospinal fluid (CSF), 2) liquefied vitreous entering through the pit or through a macular hole, and 3) leakage from either choroidal vessels or permeable vessels in the pit.  Optic pits are not associated with brain malformations – so they do not warrant neuroimaging.
  • 30. Treatment The treatment of serous macular detachment associated with an optic disc pit is still controversial.  Observation: spontaneous resolution has been seen in 25% cases.  Laser photocoagulation: creating a barrier of chorioretinal adhesions at the temporal optic disc border but repeated treatments may be required.  Gas tamponade with laser photocoagulation: this induces pneumatic displacement of the outer layer detachment and improves central vision.  Pars plana vitrectomy (PPV) combined with laser photocoagulation and gas tamponade: currently this approach is considered to be more effective than laser photocoagulation or gas tamponade alone, particularly in eyes with severe visual loss
  • 31. MEGALOPAPILLA  Megalopapilla is a generic term that connotes an abnormally large optic disc that lacks the inferior excavation of optic disc coloboma or the numerous anomalous features of the morning glory disc anomaly.  This condition is usually bilateral and often associated with a large cup-to-disc ratio.  Patients who have megalopapilla are often suspected to have glaucoma.  Unlike the situation in glaucoma, however, the optic cup is usually round or horizontally oval with no vertical notch or encroachment .
  • 32.
  • 33.  Visual acuity is generally normal in megalopapilla but may be mildly decreased in some cases.  Visual fields are usually normal except for an enlarged blind spot, which enables the examiner to rule out low-tension glaucoma or a compressive lesion.  Megalopapilla is only rarely associated with brain anomalies, and neuroimaging is not warranted unless midline facial anomalies are present.
  • 34. CONGENITAL TILTED DISC SYNDROME  The tilted disc syndrome is a nonhereditary bilateral condition.  The superotemporal optic disc is elevated and the inferonasal disc is displaced posteriorly, which results in an optic disc of oval appearance with its long axis obliquely orientated.  This configuration is accompanied by situs inversus of the retinal vessels, congenital inferonasal conus, thinning of the inferonasal retinal pigment epithelium and choroid, and myopic astigmatism.  These features presumably result from a generalized ectasia of the inferonasal fundus that involves the corresponding sector of the optic disc.
  • 35.
  • 36. (A) Tilted disc; (B) tilted disc and inferonasal chorioretinal thinning
  • 37.  Familiarity with this condition is important because affected patients may present with the suggestion of bitemporal hemianopias, which involve primarily the superotemporal quadrants.  However, these field defects, when observed carefully, do not respect the vertical meridian (as do chiasmal lesions).  Furthermore, large and small isopters are fairly normal, but medium-sized isopters are constricted selectively because of the ectasia of the midperipheral fundus.
  • 38.  Repeated visual field tests after correcting for the myopic refractive error often eliminate the field defect, which confirms its refractive nature.  In some cases, retinal sensitivity is decreased in the area of the ectasia, which causes the defect to persist despite refractive correction.  Rare cases of the tilted disc syndrome have been documented in patients who have congenital suprasellar tumors; neuroimaging is therefore warranted when the associated bitemporal hemianopia respects the vertical meridian.
  • 39. CONGENITAL OPTIC DISC PIGMENTATION  Congenital optic disc pigmentation is a condition in which melanin anterior to or within the lamina cribrosa imparts a gray appearance to the disc.
  • 40.  True congenital optic disc pigmentation is extremely rare.  Congenital optic pigmentation is compatible with good visual acuity but may be associated with coexistent optic disc anomalies that decrease vision.  Most cases of gray optic discs are not caused by congenital optic disc pigmentation.  For reasons that are understood poorly, optic discs of infants who have delayed visual maturation or albinism and those of some normal neonates have a diffuse gray tint when viewed ophthalmoscopically.  In these disorders, the gray tint disappears within the first year of life without visible pigment migration.

Notas del editor

  1. ONH is seen ophthalmoscopically as an abnormally small optic nerve head which may or may not accompany periventricular leucomalacia (PVL).
  2. It needs to be distinguished from the other congenital disc lesions, especially optic nerve coloboma (ONC) and peripapillary staphyloma. Ophthalmoscopically, the two entities are distinct - the morning glory disc lies symmetrically and centrally within the excavation, whereas in ONC the excavation lies aymmetrically, and usually inferiorly within the optic disc (Table 1).