Skip to main content

Curie temperature of weakly shocked target basalts at the Lonar impact crater, India


The study investigates Curie temperature (TC), bulk magnetic susceptibility, hysteresis, and X-ray diffraction pattern of in situ target basalts of Lonar impact crater, India. The main magnetic phase in the target basalt is low-Ti titanomagnetite. This study reveals an increase in TC and decrease in magnetic susceptibility and in full width at half maxima of the 311 peaks of titanomagnetite with distance from the crater center. Changes in crystal lattice of titanomagnetite, such as straining of 311 peaks, decrease in apparent crystallite size, and grain fragmentation may be among the possible reasons for the observed trends in TC and magnetic susceptibility. However, they both do not show any correlation between each other, indicating that different shock-induced processes affect them.


Magnetite is a common ferrimagnetic mineral in the terrestrial and extraterrestrial rocks. Magnetite and other ferromagnetic minerals are a source of magnetic anomalies associated with terrestrial and extraterrestrial impact craters and, therefore, play an important role in their discovery and mapping (e.g., Pilkington and Grieve 1992; Plado et al. 1999; Gilder et al. 2018). Moreover, behavior of magnetite and other ferromagnetic minerals at various shock pressures has been used to identify the magnetic mineralogy of Mars (Louzada et al. 2011). Although critical for impact cratering research on Earth and elsewhere, the behavior of magnetite, in weakly shocked rocks, is not well understood.

Magnetite has a typical inverse spinel structure with Fe(II) and Fe(III) disordered in the octahedral sites and fully occupied tetrahedrons by Fe(III) cation (Verwey and Haayman 1941). At temperatures below Verwey transition (TV), about 110–120 K, magnetite has an orthorhombic crystal structure (Verwey and Haayman 1941; Iizumi et al. 1982). At temperatures between TV and Curie temperature—TC (~ 856 K or 582.85 °C), it is cubic, and it is ferrimagnetic due to an anti-ferromagnetic coupling of Fe(III) in tetrahedral and octahedral sites and Fe(II) in octahedral sites (Néel 1948; Tarling and Hrouda 1993). Beyond TC, it is paramagnetic (Shull et al. 1951), due to the loss of magnetic ordering (Harrison and Putnis 1995, 1996).

Titanomagnetites form a solid-solution series (Fe3-xTixO4) with magnetite (0 = x) and ulvöspinel (x = 1) as the two end members. The dependence of magnetite TC upon the chemical composition is well established. There is a negative correlation between TC and the ulvöspinel content, ‘x’ (e.g., Akimoto et al. 1957; Özdemir and O’Reilly 1981; Moskowitz et al. 1998; Lattard et al. 2006). This correlation is owed to the change in lattice parameters due to replacement of Fe cation by Ti (Akimoto et al. 1957).

Another factor affecting TC is hydrostatic pressure. TC of titanomagnetite, with ulvöspinel component from 0 to 0.7, increases linearly with static pressures up to 6 GPa (Samara and Giardini 1969; Schult 1970). Under hydrostatic pressure, a cubic crystal, such as that of magnetite, results in a cubic unit cell with decreased interionic distances (barring any phase transformation). This causes increased interionic exchange and higher TC (Samara and Giardini 1969). However, a similar direct correlation between crystallographic changes and TC due to dynamic shock pressure is not yet established. This may be partly owed to lack of sufficient experimental investigations and partly due to complex shock wave behavior (reflection and refraction) due to heterogeneity in rocks at natural craters. Shock waves from natural and experimental craters may indirectly affect TC by fracturing the magnetic grains, thus facilitating hydrothermal alteration to increase the proportion of non-stoichiometric magnetite (Kontny et al. 2018). The grain fragmentation may also transform multi-domain magnetite (MD) to pseudo-single domain (PSD) or single domain (SD), thus reducing the magnetic susceptibility (e.g., Reznik et al. 2016).

This study investigates the variation in TC, magnetic susceptibility, and XRD pattern in the weakly shocked target basalts (< 3 GPa) of Lonar impact structure. The results show a systematic change in these properties with distance from the center of Lonar impact crater, i.e., with a change in peak shock pressure. To our knowledge, this is the first report of such correlation from weakly shocked rocks of a natural crater.

Geological setting and rock magnetic properties

Lonar crater (19° 58′ N, 76° 31′ E) in the Buldana district of India is a hypervelocity impact crater excavated in the ca. 65 Ma tholeiitic Deccan basalt (Hagerty and Newsom 2003; Maloof et al. 2010). Some studies using fission track and thermoluminescence dating suggested that the Lonar impact occurred 50 ka (Fredriksson et al. 1973), while other reports using 40Ar/39Ar dating argue that the impact crater is ca. 570 ka in age (Jourdan et al. 2011). The ~ 1.88 km wide simple crater is 150 m deep from the rim and is filled with a 7–10-m-deep lake. The lake is filled with 30–100-m-thick unconsolidated postimpact sediments, which are underlain by ~ 225 m of impact breccia (Fredriksson et al. 1973; Fudali et al. 1980; Grieve et al. 1989). The Lonar crater is an excellent analog of extraterrestrial impact craters on basalt. It is relatively pristine and has not undergone any postimpact tectonism (Maloof et al. 2010; Agarwal et al. 2016).

The target basalt is comprised of five very similar and homogenous Deccan basalt flows (Fig. 1), whose geochemical, textural, and rock magnetic properties have been studied in detail (e.g., Kieffer et al. 1976; Hagerty and Newsom 2003). The TiO2 content of different flows of the target basalt is similar (Osae et al. 2005). Each flow is ~ 8 to 40 m thick, separated by horizons of red and green paleosols and has vesicles filled with secondary materials like chlorite, zeolite, quartz, and brown limonite, and most have a chill margin at their bottom and a heated and brecciated top (Ghosh and Bhaduri 2003). The flows exposed in the Lonar crater wall are chemically similar and are classified as relatively low-K tholeiitic intra-plate basalts, with minor Fe and Ca enrichment and slight Mg and Al depletion compared to “average” tholeiites (Osae et al. 2005). All of the shocked basalts are altered, containing vesicles and veins full of carbonate and clays (Hagerty and Newsom 2003).

Fig. 1
figure 1

Map of Lonar crater (after Maloof et al. 2010) with sampling sites of this study. Lava flows: Tf0, Tf1, Tf2, Tf3, Tf4, Tf5, and Tf6. Coordinates are represented in UTM—WGS84

The alteration is recorded as young (< 50 kya) viscous and/or chemical remanent magnetization in the target rocks (Louzada et al. 2008; Arif et al. 2012; Agarwal et al. 2016). The target basalts also present an older component similar to the Deccan direction (Louzada et al. 2008; Agarwal et al. 2016). The main magnetic phase in the target basalt is low-Ti titanomagnetite with a magnetic domain state ranging from single to multi-domain (Agarwal et al. 2016). The target basalts exposed around the crater rim have experienced shock pressures between 0.2 and 0.5 GPa (Agarwal et al. 2016).


Shocked basalts were collected from the Lonar impact structure, India. The magnetic mineralogy was first investigated under reflected light in an optical microscope. In total, 21 samples were analyzed for the variation of magnetic susceptibility with the temperature at the Institute of Applied Geosciences, Karlsruhe Institute of Technology, Karlsruhe, Germany. The variation in low-field magnetic susceptibility at low temperature was measured with Kappabridge (KLY-4S) equipped with CS-L cryostat. The sample was cooled to − 192° C using liquid nitrogen. Then the nitrogen was flushed out using a blast of argon, and the susceptibility was measured as the sample warmed to the room temperature. For high-temperature measurements, the Kappabridge (KLY-4S) was equipped with a CS-3 furnace. The sample was heated from room temperature up to 700 °C at a rate of 10 °C/min and then cooled back. The bulk magnetic susceptibility was measured during the entire cycle of heating and cooling. Possible oxidation while heating was minimized by flushing out air from the sample holder using argon flowing at 50 ml/min. TC was calculated by two-tangent method (e.g., Petrovský and Kapička 2006). TCs thus calculated were crosschecked with the first derivative method. Bulk magnetic susceptibility of each sample was measured at room temperature in the Kappabridge (KLY-4S).

Hysteresis curves were determined using Alternating Gradient Field Magnetometer Micromag apparatus in fields up to 1.4 T. The curves allow calculating the remanence of coercivity-to-coercive force (Hcr/Hc) and the remanent magnetization-to-saturation remanence (Mrs/Ms) ratios of each sample. These ratios are used to estimate the relative proportions of the single domain (SD), multi-domain (MD), and pseudo-single domain (PSD) grains (Dunlop 2002a, b). In general, the ratio of Mrs/Ms is higher for more SD materials and lower for more MD-like materials. Agarwal et al. (2016) applied stepwise increasing uniaxial field on the samples to calculate the saturated and non-saturated isothermal remanent magnetization (IRM) acquisition curves. These curves were used to determine the median destructive field (MDF). The samples were then divided into magnetically hard, soft, and intermediate groups, based on the dominant magnetic domain state and the MDF.

The XRD pattern of magnetically hard basalts (dominated by SD) was measured with a Siemens D500 diffractometer using a Cu-Ka anode. For each sample, the 2θ range 10°–90° was scanned with an angular speed of 0.5°/min. The variation in full width at half maxima (FWHM) of the 311 peaks with distance from the crater center is calculated. This peak was selected because it is the most intense peak of the magnetite diffraction spectra and has been a subject of previous investigations as well (e.g., Reznik et al. 2016). Diffraction peaks of (Ti-)magnetite can be broadened by the reduction in crystallite size or by introducing strain into the crystal lattice (e.g., Reznik et al. 2016). The apparent crystallite size is, therefore, calculated from FWHM of the X-ray diffraction peak using Scherrer’s equation:

$$D = k\lambda /\left( {\beta \, \cos \, \theta } \right),$$

where D is the crystal diameter, k is the Scherrer’s constant (0.9 for magnetite; El Ghandoor et al. 2012), λ (0.154056 nm) is the X-ray wavelength, β the FWHM of a diffraction peak in radians, 311 in our case, and θ is the diffraction angle in radians.


Magnetic mineralogy

The basalt consists of phenocrysts of plagioclase (up to 1500 μm) in a fine-grained matrix of plagioclase (up to 60 μm,) pyroxene (up to 200 μm) and opaque phases (up to 100 μm). Reflected light microscopy reveals that most of the opaque phases are intergrown titanomagnetite and ilmenite (Fig. 3). Some grains of pyroxene and plagioclase are altered, along the fractures and grain boundaries to clay minerals.

In the thermomagnetic curves, the Verwey transition peak is broad and subtle or completely absent, indicating a minor contribution of magnetite near end-member phase (Fig. 2). However, all curves show conspicuous TC between 506 and 560 °C indicating the oxyexsolved Ti-magnetite grains with Ti-rich lamellae in a Ti-depleted host (e.g., Jackson and Bowles 2014), which is also supported by reflected light microscopic observation (Fig. 3a). A second TC is common in the heating branch between 300 and 450 °C, possibly indicating Ti-maghemite (e.g., Moskowitz 1981). The curves are generally reversible over 500–550 °C (Fig. 2). In the cooling branch, the absence of the second TC and lower susceptibility and the irreversibility below 500 °C are owed to the destruction of Ti-maghemite possibly into Ti-hematite at high temperatures (e.g., Alva-Valdivia et al. 2017, 2019).

Fig. 2
figure 2

Representative χ-T curves of the basalts showing the variation in magnetic susceptibility during heating (black) and cooling (gray). The higher TC is marked by a black arrow. AU arbitrary units

Fig. 3
figure 3

Reflected light photomicrographs present a oxyexsolved Tmt grains with Ti-rich lamellae and b an optically homogeneous titanomagnetite (Tmt) grains

The Hcr/Hc ratio varies from 0.174 to 2.672 and the Mrs/Ms ratio varies from 0.04 to 0.373, indicating that the magnetic behavior in different samples is dominated by different domain states ranging from SD to MD. Depending upon the dominant magnetic domain state and the MDF of the remanence (varying from 6 to 61 mT), the target basalts were divided into three groups: (Group 1) thirteen samples dominated by SD and presenting a magnetically hard behavior with MDF > 22 mT; (Group 2) five magnetically soft samples dominated by MD with MDF ≤ 7 mT; and (Group 3) three intermediate samples with a mixture of SD and MD, and MDF between 8 and 21 mT.

Shock effects

The basalts of Group 1 (with high MDF and dominated by SD) show a clear increase in TC with distance from the crater center, i.e., decreasing shock pressure (Fig. 4). Notably, TC increases from 475.6 °C to 562 °C almost linearly. Basalts of Group 2 and 3 show a similar increase in TC with distance from the crater center (Additional file 1: Figure S1). However, due to fewer samples (5 and 3, respectively) and statistically unreliable trend, they are excluded from further investigations.

Fig. 4
figure 4

Variation in TC, bulk magnetic susceptibility and FWHM with the distance from the crater center. Note that the black trend line is calculated by excluding sample 8

Contrary to this trend of TC, the bulk magnetic susceptibility and the FWHM of the group 1 basalt decrease with distance from the crater center (Fig. 4). The bulk magnetic susceptibility decreases from 75.3 × 10−3 SI to 46.8 × 10−3 SI, while the 2θ of the FWHM decreases from 0.43° to 0.24° (Table 1). The apparent crystal diameter ‘D’ increases with distance from the crater center in accordance with the FWHM. For sample 34, nearest to the crater center, D is 21.53 nm, while for sample 11, which is farthest from the crater center, D is 35.38 nm (Table 1).

Table 1 Table compiles the distance of each sample from the crater center; apparent crystallite size is (D); bulk magnetic susceptibility (χ); Curie temperature (TC); the ratios: remanence of coercivity to coercive force (Hcr/Hc) and the remanent magnetization to saturation remanence (Mrs/Ms)

Note that, sample 8, collected from the north of the Lonar crater, it is farthest from the crater, but presents the least TC (475.6 °C). This sample is an outlier to all these trends and is excluded during calculating the trend line and from further discussion.


The study reports magnetic mineralogy, bulk magnetic susceptibility and the XRD pattern of shocked basalts from the Lonar impact structure, India. In the shocked basalts, TC decreases but the FWHM of the 311 peak and bulk magnetic susceptibility increase with vicinity to the crater center, i.e., with increasing shock pressures (Fig. 4, Additional file 1: Fig. S1).

The increase in FWHM with vicinity to the crater center may be owed to increasing strain in the crystal lattice, due to anisotropic compression by shock waves, and to decreasing apparent crystallite size (e.g., Reznik et al. 2016). The crystallite size of shocked magnetite reported here for Lonar basalts (21.3–35.38 nm) is smaller than the size (80–180 nm) reported by Reznik et al. (2016). This difference may be due to the fact that the starting material for Reznik et al. (2016) was of the banded magnetite-quartz ore with larger unshocked crystals, whereas in Lonar basalts, magnetite is an accessory mineral with smaller crystals.

Variation in bulk magnetic susceptibility

The target basalts at Lonar impact structure present an increase in bulk susceptibility with increasing shock pressure. On the one hand, these trends disagree with the effects of static pressures up to 0.6 GPa, which decrease the bulk magnetic susceptibility (Kapička 1988). The decrease is owed to significant isomer shifts that octahedral lattices of magnetite undergo up to 5 GPa (Halasa et al. 1974), and to linear volume decrease possibly causing anisotropic compression, thus influencing the magnetic lattice network via changes in magnetostriction and magnetocrystalline constants (Nagata and Kinoshita 1967; Gilder et al. 2004).

On the other hand, present observations agree with the trends in cratering experiments. Here experimental shock pressure (< 3 GPa) increases the bulk magnetic susceptibility of rocks with small magnetite grains, < 10 µm (Agarwal et al. 2019). Although the mechanism behind this increase is not known, their results agree well with the present observations. In contrast, at higher shock pressures (3–20 GPa), bulk magnetic susceptibility decreases due to damage in the crystal lattice and grain fragmentation causing MD magnetite to break into PSD and SD magnetite (Nishioka et al. 2007; Louzada et al. 2010; Reznik et al. 2016, 2017). A decrease in magnetic susceptibility is also reported from the drill cores of the El’gygytgyn impact structure but is owed to impact-related hydrothermal alteration (Kontny and Grothaus 2017).

Variation in Curie temperature

The decrease in TC with increasing shock pressure in Lonar basalts is in contrast to the effects of static pressure. For example, static pressures up to 5 GPa are known to increase TC (Schult 1970). The changes in the crystal lattice by shock waves may affect the TC. However, no other natural and experimental studies have investigated the effect of dynamic pressures on TC and therefore a comparison is not possible.

Notably, changes in TC and magnetic susceptibility due to formation of new magnetite (by hydrothermal alteration or some other process) may be precluded because paleomagnetic investigations reveal a single high coercivity component, which is associated with the emplacement of the basalts (Louzada et al. 2008; Agarwal et al. 2016). The scatter in the trends of TC and magnetic susceptibility (Fig. 4) could be related to slight variation in magnetic mineralogy that predates impact or could arise from heterogeneity in the pressure field at the time of impact.


Until now, the shock demagnetization of magnetic minerals such as magnetite, Ti-magnetite, hematite, Ti-hematite, and pyrrhotite (see Louzada et al. 2011 and the references therein) was the only effect of low shock pressures (< 3 GPa), which was considered of importance at a regional scale. However, now, increase in magnetic susceptibility of Ti-magnetite, at low shock pressures, is clear from present investigations on naturally shocked target basalts at Lonar impact structure, and from experiments (Agarwal et al. 2019). As most of the target rocks in the crater subsurface are generally weakly shocked, < 3 GPa (Pierazzo and Melosh 2000; Kenkmann et al. 2014), such an increase in magnetic susceptibility will affect the induced magnetization, thus, changing the magnetic anomalies at these impact structures.

While there are no other studies on the TC of weakly shocked rocks, there is only one study on magnetic susceptibility, which shows its increase with shock pressures below 3 GPa, without commenting on the mechanism (e.g., Agarwal et al. 2019). Changes in the crystal lattice, such as straining of (311) peak, decrease in apparent crystallite size, and grain fragmentation may be among the possible reasons for one of the observed trends in TC and magnetic susceptibility. However, they both do not show any correlation between each other, indicating that different shock-induced processes affect them.

Moreover, the deformation under static and dynamic condition is fundamentally different because of phenomenon like strain hardening (Simpson 1985). Studies on the effects of experimental and natural static pressures, therefore, cannot directly be used to interpret the effects of dynamic shock waves. The present data set reveals systematic changes in TC and magnetic susceptibility with shock pressures below 3 GPa. However, the present data do not pin down the precise mechanism behind these changes. Further experimental investigations, in controlled settings, which link rock magnetic changes with crystallographic effects at low shock pressures are needed to identify the active processes.

Availability of data and materials

All of the data on which this manuscript is based are provided in the main text.


Download references


Phillip Lied measured the thermomagnetic curves. Prof. A. Kontny is thanked for access to the Kappabridge. We thank two anonymous reviewers for their helpful constructive criticism and the editors for their guidance during the review process.


The fieldwork was funded by Deutscher Akademischer Austauschdienst (A/11/76052) and by Innovationsfonds 2017 Uni Freiburg. AA holds the Alexander von Humboldt Post-Doctoral Fellowship.

Author information

Authors and Affiliations



AA collected the samples and interpreted the thermomagnetic and XRD results. LM measured and interpreted hysteresis. Both authors read and approved the final manuscript.

Corresponding author

Correspondence to A. Agarwal.

Ethics declarations

Competing interests

The authors declare that they have no competing interests.

Additional information

Publisher's Note

Springer Nature remains neutral with regard to jurisdictional claims in published maps and institutional affiliations.

Supplementary information

Additional file 1: Figure S1.

Variation in Curie temperature with the distance from the crater center for Group 2 (Low coercivity—Soft) and Group 3 (Intermediate coercivity) samples.

Rights and permissions

Open Access This article is licensed under a Creative Commons Attribution 4.0 International License, which permits use, sharing, adaptation, distribution and reproduction in any medium or format, as long as you give appropriate credit to the original author(s) and the source, provide a link to the Creative Commons licence, and indicate if changes were made. The images or other third party material in this article are included in the article's Creative Commons licence, unless indicated otherwise in a credit line to the material. If material is not included in the article's Creative Commons licence and your intended use is not permitted by statutory regulation or exceeds the permitted use, you will need to obtain permission directly from the copyright holder. To view a copy of this licence, visit

Reprints and Permissions

About this article

Verify currency and authenticity via CrossMark

Cite this article

Agarwal, A., Alva-Valdivia, L.M. Curie temperature of weakly shocked target basalts at the Lonar impact crater, India. Earth Planets Space 71, 141 (2019).

Download citation

  • Received:

  • Accepted:

  • Published:

  • DOI:


  • Lonar impact crater
  • Variation in Curie temperature
  • Variation in bulk magnetic susceptibility
  • X-ray diffraction pattern