| Literature DB >> 28584270 |
Thomas Raap1, Rianne Pinxten2,3, Giulia Casasole2, Nina Dehnhard2, Marcel Eens2.
Abstract
Urbanization is associated with dramatic increases in noise and light pollution, which affect animal behaviour, physiology and fitness. However, few studies have examined these stressors simultaneously. Moreover, effects of urbanization during early-life may be detrimental but are largely unknown. In developing great tits (Parus major), a frequently-used model species, we determined important indicators of immunity and physiological condition: plasma haptoglobin (Hp) and nitric oxide (NOx) concentration. We also determined fledging mass, an indicator for current health and survival. Associations of ambient noise and light exposure with these indicators were studied. Anthropogenic noise, light and their interaction were unrelated to fledging mass. Nestlings exposed to more noise showed higher plasma levels of Hp but not of NOx. Light was unrelated to Hp and NOx and did not interact with the effect of noise on nestlings' physiology. Increasing levels of Hp are potentially energy demanding and trade-offs could occur with life-history traits, such as survival. Effects of light pollution on nestlings of a cavity-nesting species appear to be limited. Nonetheless, our results suggest that the urban environment, through noise exposure, may entail important physiological costs for developing organisms.Entities:
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Year: 2017 PMID: 28584270 PMCID: PMC5459827 DOI: 10.1038/s41598-017-02940-5
Source DB: PubMed Journal: Sci Rep ISSN: 2045-2322 Impact factor: 4.379
Average noise levels in our study population. Average noise levels are given per year.
| Year | Average noise (dB) ± SE | N |
|---|---|---|
| 2012 | 51.5 ± 0.6 | 69 |
| 2013 | 54.3 ± 0.8 | 74 |
| 2014 | 53.4 ± 0.8 | 84 |
| 2015 | 53.1 ± 0.8 | 79 |
Sample sizes (N) varied between years but consisted mostly of the same nests, with 67 nests being measured in all four years.
Noise measurements in our study population are highly correlated over the years.
| 2012 | 2013 | 2014 | |
|---|---|---|---|
|
| 0.69 | ||
|
| 0.61 | 0.66 | |
|
| 0.54 | 0.52 | 0.57 |
Spearman rank correlation coefficient (adjusted for multiple tests; Holm correction) are given for nightly noise measurements between 2012–2015. All correlations were significant (P < 0.001).
Results of the fledging mass, Hp and NOx model selection procedure based on AICc.
| AICc | ∆ AICc | Akaike weight | |
|---|---|---|---|
|
| |||
| s | 1834.9 | 0 | 0.622 |
| light + s | 1835.9 | 1 | 0.378 |
|
| |||
| b + ld + s + noise + light + light:s | 2651.3 | 0.00 | 0.093 |
| b + s + light + noise + light:s + noise: light | 2651.3 | 0.07 | 0.090 |
| b + ld + s + light + noise + light:s + noise: light | 2651.6 | 0.38 | 0.077 |
| ld + s + light + noise + light:s | 2651.7 | 0.44 | 0.074 |
| b + s + light + noise + light:s | 2651.9 | 0.60 | 0.069 |
| b + ld + s + light + noise | 2651.9 | 0.60 | 0.069 |
| b + ld + s + noise | 2652.1 | 0.81 | 0.062 |
| b + s + light + noise + noise: light | 2652.3 | 1.06 | 0.055 |
| ld + s + light + noise | 2652.4 | 1.11 | 0.053 |
| b + s + light + noise | 2652.4 | 1.18 | 0.052 |
| b + ld + light + noise | 2652.6 | 1.35 | 0.047 |
| b + ld + s + light + noise + noise: light | 2652.6 | 1.38 | 0.047 |
| ld + s + noise | 2652.7 | 1.44 | 0.045 |
| b + s + noise | 2652.7 | 1.47 | 0.045 |
| ld + s + light + noise + light:s + noise: light | 2652.8 | 1.50 | 0.044 |
| b + ld + noise | 2652.8 | 1.52 | 0.044 |
| ld + light + noise | 2653.2 | 1.93 | 0.035 |
|
| |||
| fledging mass | 612.8 | 0 | 0.73 |
| fledging mass + s | 614.8 | 1.99 | 0.27 |
Linear mixed models with “NestID” as random factor were used to avoid pseudoreplication. Top ranked models included noise in combination with sex (s), light, brood size (b), laying date (ld), fledging mass, the interaction light:sex (light:s) and/or the interaction noise:light. Fledging mass models were run on data from 562 nestlings from 85 nests; Hp models on data from 475 nestlings from 78 nests and NOx models on data from 344 nestlings from 58 nests. Only models within ∆ AICc < 2 of the top model are shown.
Results from the Hp model selection procedure showing parameter estimates and selection probabilities (see Statistical analysis and Table 2).
| Parameter | Estimate ± SE | RVI | Effect size |
|---|---|---|---|
| Brood size | 0.46 ± 0.20 | 0.75 | 0.059 |
| Laying date | −0.12 ± 0.04 | 0.69 | 0.072 |
| Sex | −0.69 ± 0.38 | 0.87 | 0.008 |
| Light | −8.54 ± 12.47 | 0.80 | 0.044 |
| Noise | 0.20 ± 0.06 | 1.00 | 0.116 |
| Light:Sex | 0.83 ± 1.41 | 0.45 | 0.001 |
| Noise:Light | 0.35 ± 0.19 | 0.31 | 0.043 |
Only factors that were used for model averaging are shown. Models were run on data from 475 nestlings of 78 nests. Haptoglobin levels had been square root transformed. Relative variable importance (RVI) are shown as well as effect sizes (partial R ’s) which were calculated following Edwards, et al.[74].
Figure 1Nestlings exposed to higher levels of noise had higher levels of haptoglobin. Raw data of average Hp concentration per nest (square root transformed) in response to measured noise levels at the nest entrance. Lines represent model-averaged estimate and 95% confidence intervals (see Statistical analysis and Tables 2 and 3; partial R = 0.116), based on data from 475 nestlings of 78 nests.