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4D Imaging of Protein Aggregation in Live Cells
* These authors contributed equally
Biology
Summary
Cellular viability depends on timely and efficient management of protein misfolding. Here we describe a method for visualizing the different potential fates of a misfolded protein: refolding, degradation, or sequestration in inclusions. We demonstrate the use of a folding sensor, Ubc9ts, for monitoring proteostasis and aggregation quality control in live cells using 4D microscopy.
Cite this Article
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Spokoini, R., Shamir, M., Keness, A., Kaganovich, D. 4D Imaging of Protein Aggregation in Live Cells. J. Vis. Exp. (74), e50083, doi:10.3791/50083 (2013).
Abstract
One of the key tasks of any living cell is maintaining the proper folding of newly synthesized proteins in the face of ever-changing environmental conditions and an intracellular environment that is tightly packed, sticky, and hazardous to protein stability1. The ability to dynamically balance protein production, folding and degradation demands highly-specialized quality control machinery, whose absolute necessity is observed best when it malfunctions. Diseases such as ALS, Alzheimer's, Parkinson's, and certain forms of Cystic Fibrosis have a direct link to protein folding quality control components2, and therefore future therapeutic development requires a basic understanding of underlying processes. Our experimental challenge is to understand how cells integrate damage signals and mount responses that are tailored to diverse circumstances.
The primary reason why protein misfolding represents an existential threat to the cell is the propensity of incorrectly folded proteins to aggregate, thus causing a global perturbation of the crowded and delicate intracellular folding environment1. The folding health, or "proteostasis," of the cellular proteome is maintained, even under the duress of aging, stress and oxidative damage, by the coordinated action of different mechanistic units in an elaborate quality control system3,4. A specialized machinery of molecular chaperones can bind non-native polypeptides and promote their folding into the native state1, target them for degradation by the ubiquitin-proteasome system5, or direct them to protective aggregation inclusions6-9.
In eukaryotes, the cytosolic aggregation quality control load is partitioned between two compartments8-10: the juxtanuclear quality control compartment (JUNQ) and the insoluble protein deposit (IPOD) (Figure 1 - model). Proteins that are ubiquitinated by the protein folding quality control machinery are delivered to the JUNQ, where they are processed for degradation by the proteasome. Misfolded proteins that are not ubiquitinated are diverted to the IPOD, where they are actively aggregated in a protective compartment.
Up until this point, the methodological paradigm of live-cell fluorescence microscopy has largely been to label proteins and track their locations in the cell at specific time-points and usually in two dimensions. As new technologies have begun to grant experimenters unprecedented access to the submicron scale in living cells, the dynamic architecture of the cytosol has come into view as a challenging new frontier for experimental characterization. We present a method for rapidly monitoring the 3D spatial distributions of multiple fluorescently labeled proteins in the yeast cytosol over time. 3D timelapse (4D imaging) is not merely a technical challenge; rather, it also facilitates a dramatic shift in the conceptual framework used to analyze cellular structure.
We utilize a cytosolic folding sensor protein in live yeast to visualize distinct fates for misfolded proteins in cellular aggregation quality control, using rapid 4D fluorescent imaging. The temperature sensitive mutant of the Ubc9 protein10-12 (Ubc9ts) is extremely effective both as a sensor of cellular proteostasis, and a physiological model for tracking aggregation quality control. As with most ts proteins, Ubc9ts is fully folded and functional at permissive temperatures due to active cellular chaperones. Above 30 °C, or when the cell faces misfolding stress, Ubc9ts misfolds and follows the fate of a native globular protein that has been misfolded due to mutation, heat denaturation, or oxidative damage. By fusing it to GFP or other fluorophores, it can be tracked in 3D as it forms Stress Foci, or is directed to JUNQ or IPOD.
Protocol
1. Yeast Preparations
1. Transform yeast strains with a plasmid carrying a GAL1-GFP-Y68L (UBC9ts) cassette.
2. Grow yeast in synthetic media containing 2% raffinose for 24 hr and back diluted to 2% galactose containing media for 16 hr or O/N. Incubate cells at 30 °C while shaking at 200 rpm.
3. The following morning, dilute the query strain to OD600= 0.2. Shake for 4-6 hr at 30 °C (200 rpm) until the culture reaches OD600= 0.8-1.0.
4. To repress expression (so as to monitor only the already-translated and folded pool of GFP-Ubc9ts), change media to synthetic media supplemented with 2% glucose (SD) 30 min prior to imaging.
5. Treatment - Heat shock the cells for 20 min at 37 °C to induce misfolding, or continuously in microscope incubator to follow protein aggregation in heat-shock conditions. Note - if you are using the microscope at any temperature above RT, pre-heat for about 2 hr to equilibrate the temperature along the body of the microscope and the objectives (see below).
2. Plate\Slide Preparations
1. Choose appropriate plate. The main consideration is the ability to maintain focus during imaging acquisition. The following points are critical for 4D imaging and not for 2D time lapses or 3D imaging.
1. Multiple wells plate- the bottom of the different wells may not be homogenous (i.e. the wells will be at different heights relative to the objective). This will make it difficult to maintain focus across x y points and time points, regardless of the autofocusing technique being used.
2. Slide material: glass vs. plastic. Glass bottomed slides are more z-homogenous between wells, but are more expensive.
3. Thickness of the plate's bottom: we usually use coverslip-bottom plates index 1.5, but index 1 is also acceptable depending on the objective.
2. Cover bottom of the plate\slide with ConA (0.25 mg/ml) for 10 min. ConA is used to adhere cells to the slide, which enables following a single cell over time.
3. Remove ConA and incubate the slide in a chemical hood so that excess ConA will evaporate.
4. Plate 200 μl of yeast sample (OD600= 0.5) into the ConAed well.
5. Incubate for 15 min, as to enable cells stick to the surface of the plate.
6. Extract the medium, and wash three times with new medium to get one layer of cells. Note: if a long time lapse is planned, seed the cells sparsely so that new buds won't fill and interrupt the region of interest.
3. Microscope Preparations
1. We use a Nikon A1Rsi confocal microscope with a few non-standard modifications. For yeast imaging we use up to 4 lasers (405 nm, 50 mW CUBE laser; 457-514 nm, 65 mW Argon Ion laser; 561 nm, 50 mW Sapphire laser; and 640 nm, 40 mW CUBE laser), and up to 4 PMTs equipped with filters. Most of our imaging is done with a green filter set for EGFP and a red filter set for mCherry and tdTomato. With GFP and mCherry there is almost no bleedthrough, therefore we often use simultaneous scanning. However, line-scanning can also be used to prevent bleedthrough when it does occur. Our confocal is also equipped with a PInano Piezo stage (MCL), which can make 3 msec steps in z, enabling 2-3 z-stacks (30-50 sections) per second. The systems also has a spectral detector, Perfect Focus (laser offset), and two scanners - a galvano scanner and a resonant scanner.
2. Choose appropriate objective. Main considerations:
1. Water/Oil/Air objective: the main consideration is the refractive index of the imaging medium vs the medium of the sample.
1. Oil objective advantages:
1. Oil objectives can have higher numerical apertures (oil breaks light more than water, and therefore more photons go back to the objective). Oil objectives can have up to NA 1.49, compared to 1.27 for water. (However, this is not actually a huge difference in resolution).
2. The refractive index of oil matches the refractive index of glass, therefore no photons are lost going from the sample, through the glass, to the objective. (Note - chose an immersion oil that has a refractive index that is appropriate for your objective and your coverslip).
3. Oil enables hassle-free long time-lapses since it does not evaporate.
Oil Objective disadvantages:
1. The higher resolution enabled by the higher NA of oil objectives degrades rapidly if the light has to travel through an aqueous medium (such as a cell).
2. Images typically have more spherical aberrations and a "stretched out" effect in 3D.
3. Oil is sticky, messy, and a hazard to objectives.
2. Water objective advantages
1. The cell itself is aqueous, therefore there are fewer distortions in z, and the resolution remains high deep into an aqueous sample.
2. Clean and user friendly. Water objective disadvantages: evaporates quickly, therefore not suitable for long movies without special arrangements being made to pump water continuously to the objective.
3. Air objective advantages: 1. No material is lost/evaporates during multiple point acquisition or a long movie. 2. Clean and user friendly. Disadvantage: low resolution and low signal sensitivity.
2. Room and incubator temperature: changing temperature affects matter properties, and in delicate systems changes the focus. The temperature should be adjusted before choosing points for acquisition. Changing the temperature during acquisition will disrupt imaging and will result in loss of focus. We let our microscope system equilibrate for 2 hr at the desired temperature before imaging.
3. Correction collars: Many objectives come with a correction ring enabling the objective to be adjusted for a given cover-slip thickness. We recommend adjusting the correction collar while using fluorescent beads to visualize the point spread function. This will ensure correct settings for every sample.
4. Stable sample holders: we find that most commercially available sample holders are the weakest part of the microscope. They are often wobbly and not straight. This is a disaster for high-resolution, multi-point 4D imaging. We design our own sample holders that are straight and fit tightly onto the stage. They can also be bolted down when needed.
5. Multi-point acquisition: our imaging system is equipped with the Nikon "Perfect focus" system, which is basically a laser-based auto-focus mechanism. However, autofocusing is not necessarily necessary with 4D imaging, especially if the system does not drift a lot.
4. Imaging
1. Turn on the system: lasers, stage, controller, camera and computer software.
2. Place plate on stage holder, properly secured and stabilized.
3. Use eye port to determine location and orientation of yeast.
4. Using brightfield, assess cell health and viability according to shape and texture.
5. Turn on epifluorescent light according to the relevant fluorophore (e.g. FITC filter for GFP), and focus on cells displaying the phenotype which is subject to your research. Cells which are highly fluorescent in more than one wavelength may be dead and therefore autofluorescent. We visualize the nucleus with a tdTomato fluorophore fused to an SV40 NLS signal (NLS-TFP). TFP is twice the size of GFP, and is therefore above the diffusion limit of the nucleus, therefore it works very well as a nuclear marker. We can also excite TFP with a green (488 nm) laser simultaneously as GFP, but collect the green and red emissions into two separate PMTs for spectral resolution.
6. Adjust the following settings to minimize noise and oversaturation:
1. Laser power - photobleaching and phototoxicity vs. brightness of image should be considered.
2. Gain: affects camera sensitivity, thus Signal to Noise ratio.
3. Pinhole diameter - should be adjusted according to the laser with the shorter wavelength. The pinhole diameter determines the thickness (height) of the optical section imaged. Thus, opening the pinhole will collect more light (let more photons in), but will decrease resolution in z (less confocality).
7. Useful tips:
1. If different fluorophores emit congruent wavelength, use the Spectral Detector feature which enables the choice of virtual filters. Keep in mind that spectral detectors are less sensitive than regular PMTs.